This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461136.6350,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AG Mon 20260406.1350 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461136.6350,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260406.1350 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.5215-03.5259,2461136.6350,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.5215-03.5259 20260406.1350 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114330784049156736,2461136.6350,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114330784049156736 20260406.1350 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.5325-04.3524,2461136.6350,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.5325-04.3524 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109235166132314112,2461136.6350,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109235166132314112 20260406.1350 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0702018-021634,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0702018-021634 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
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 06.1350 2461136.6350 13.48 07:13:26.54 +00:56:15.8
214.60909 5.32296 galactic Mon Second-epoch detections are separated by 1.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 varaible 3111404365131719296 | 07:13:26.54 +00:56:15.8 (user input) | DSCT/GDOR/SXPHE (Gaia DR3) | 2022yCat.1358....0G | (position from user input) Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F2 (LAMOST DR5) J-Ks=0.182+/-0.043 (F)
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 3111404365131719296,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 3111404365131719296 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.5786-04.1534,2461136.6350,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.5786-04.1534 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8482-01.3642,2461136.6350,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8482-01.3642 20260406.1350 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9462+01.7102,2461136.6350,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.9462+01.7102 20260406.1350 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108790478098341120,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108790478098341120 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8884-01.1768,2461136.6350,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.8884-01.1768 20260406.1350 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9779+02.9024,2461136.6350,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9779+02.9024 20260406.1350 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111917630903223296,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111917630903223296 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108267183586677120,2461136.6350,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108267183586677120 20260406.1350 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2286+00.4776,2461136.6350,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2286+00.4776 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127775062478075136,2461136.6350,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127775062478075136 20260406.1350 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107637197783360768,2461136.6350,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107637197783360768 20260406.1350 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112803528038358144,2461136.6350,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112803528038358144 20260406.1350 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0316+00.7824,2461136.6350,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.0316+00.7824 20260406.1350 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5830+01.1318,2461136.6350,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5830+01.1318 20260406.1350 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.7633-03.3640,2461136.6350,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.7633-03.3640 20260406.1350 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110002693968004224,2461136.6350,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110002693968004224 20260406.1350 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109606113865803136,2461136.6350,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109606113865803136 20260406.1350 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115595497299893376,2461136.6350,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115595497299893376 20260406.1350 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110951018447534464,2461136.6350,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110951018447534464 20260406.1350 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.3811-01.6401,2461136.6350,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.3811-01.6401 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9388-05.7085,2461136.6350,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9388-05.7085 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110211017060985344,2461136.6350,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110211017060985344 20260406.1350 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4047+02.1260,2461136.6350,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4047+02.1260 20260406.1350 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8508-00.6575,2461136.6350,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8508-00.6575 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.2470+00.8525,2461136.6350,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.2470+00.8525 20260406.1350 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.4939-02.0083,2461136.6350,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.4939-02.0083 20260406.1350 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119367470718089088,2461136.6350,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119367470718089088 20260406.1350 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4191-04.3825,2461136.6350,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4191-04.3825 20260406.1350 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6002-04.1912,2461136.6350,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6002-04.1912 20260406.1350 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3714+02.4068,2461136.6350,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3714+02.4068 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115944351723923584,2461136.6350,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115944351723923584 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2008+01.3366,2461136.6350,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2008+01.3366 20260406.1350 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107947977311377408,2461136.6350,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107947977311377408 20260406.1350 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110390615412571392,2461136.6350,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110390615412571392 20260406.1350 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109500251512786944,2461136.6350,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109500251512786944 20260406.1350 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115543300556247680,2461136.6350,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115543300556247680 20260406.1350 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.3712-04.1472,2461136.6350,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.3712-04.1472 20260406.1350 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108383555718321408,2461136.6350,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108383555718321408 20260406.1350 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.0789-01.5704,2461136.6350,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.0789-01.5704 20260406.1350 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108824601619113600,2461136.6350,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108824601619113600 20260406.1350 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111146838894036224,2461136.6350,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111146838894036224 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107648841428697088,2461136.6350,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107648841428697088 20260406.1350 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109199054047735936,2461136.6350,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109199054047735936 20260406.1350 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8650-01.8472,2461136.6350,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.8650-01.8472 20260406.1350 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110105738822752256,2461136.6350,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110105738822752256 20260406.1350 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107892555054513664,2461136.6350,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107892555054513664 20260406.1350 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4262-03.9278,2461136.6350,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.4262-03.9278 20260406.1350 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127192493115969152,2461136.6350,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127192493115969152 20260406.1350 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115696446209927808,2461136.6350,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115696446209927808 20260406.1350 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059600153239450368,2461136.6350,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059600153239450368 20260406.1350 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7633-01.7514,2461136.6350,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.7633-01.7514 20260406.1350 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111562385568206208,2461136.6350,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111562385568206208 20260406.1350 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7880+00.3137,2461136.6350,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7880+00.3137 20260406.1350 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2155-02.4511,2461136.6350,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2155-02.4511 20260406.1350 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109834090734245504,2461136.6350,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109834090734245504 20260406.1350 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110294236346089344,2461136.6350,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110294236346089344 20260406.1350 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.2190-04.5421,2461136.6350,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.2190-04.5421 20260406.1350 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2021+00.7657,2461136.6350,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2021+00.7657 20260406.1350 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108223855955962368,2461136.6350,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108223855955962368 20260406.1350 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111297540705533952,2461136.6350,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111297540705533952 20260406.1350 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112760647085290752,2461136.6350,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112760647085290752 20260406.1350 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059210719964348544,2461136.6350,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059210719964348544 20260406.1350 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107988968482458496,2461136.6350,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107988968482458496 20260406.1350 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7383+01.6421,2461136.6350,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7383+01.6421 20260406.1350 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.2675-03.2520,2461136.6350,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.2675-03.2520 20260406.1350 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.1350 2461136.6350 12.40 07:15:46.86 -01:58:00.5
217.46895 4.51090 galactic Mon Second-epoch detections are separated by 0.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3108324323831925632 | 07:15:44.99 -01:57:42.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 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 3108324323831925632,2461136.6350,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3108324323831925632 20260406.1350 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059463538922588672,2461136.6350,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059463538922588672 20260406.1350 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126248970398055808,2461136.6350,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126248970398055808 20260406.1350 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3058310323020763904,2461136.6350,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3058310323020763904 20260406.1350 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461136.6350,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9580+01.5948 20260406.1350 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112897600704147072,2461136.6350,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112897600704147072 20260406.1350 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.0194-01.8183,2461136.6350,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.0194-01.8183 20260406.1350 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108020308862300928,2461136.6350,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108020308862300928 20260406.1350 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8701-01.1937,2461136.6350,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.8701-01.1937 20260406.1350 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5010-02.5329,2461136.6350,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5010-02.5329 20260406.1350 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822167904956928,2461136.6350,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822167904956928 20260406.1350 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112882349279538816,2461136.6350,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112882349279538816 20260406.1350 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2021+00.7657,2461136.6350,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2021+00.7657 20260406.1350 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114422142294756608,2461136.6350,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114422142294756608 20260406.1350 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461136.6350,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6490-04.3421,2461136.6350,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6490-04.3421 20260406.1350 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3331+02.7602,2461136.6350,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3331+02.7602 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053264973402395520,2461136.6350,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053264973402395520 20260406.1350 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126395106665966080,2461136.6350,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126395106665966080 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111550355362379008,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111550355362379008 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7920-02.0410,2461136.6350,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7920-02.0410 20260406.1350 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7910+00.3663,2461136.6350,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.7910+00.3663 20260406.1350 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110150406482209152,2461136.6350,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110150406482209152 20260406.1350 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6792-01.8242,2461136.6350,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6792-01.8242 20260406.1350 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3118187144984761344,2461136.6350,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3118187144984761344 20260406.1350 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.4216+00.1163,2461136.6350,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.4216+00.1163 20260406.1350 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6670-02.7746,2461136.6350,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6670-02.7746 20260406.1350 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0511-03.7251,2461136.6350,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0511-03.7251 20260406.1350 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114813572734008832,2461136.6350,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114813572734008832 20260406.1350 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127203655728648192,2461136.6350,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127203655728648192 20260406.1350 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104844811903742208,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3104844811903742208 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.2152-03.5116,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.2152-03.5116 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7777-02.4984,2461136.6350,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7777-02.4984 20260406.1350 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059907123139873664,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059907123139873664 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0649169-063043,2461136.6350,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0649169-063043 20260406.1350 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3061678195853858304,2461136.6350,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3061678195853858304 20260406.1350 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3368+02.0374,2461136.6350,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3368+02.0374 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114325664447971712,2461136.6350,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114325664447971712 20260406.1350 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127217163407760640,2461136.6350,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127217163407760640 20260406.1350 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461136.6350,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126271617766100608 20260406.1350 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4580+02.5742,2461136.6350,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4580+02.5742 20260406.1350 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059163063009453312,2461136.6350,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059163063009453312 20260406.1350 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0342-03.0807,2461136.6350,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.0342-03.0807 20260406.1350 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114877172608642176,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114877172608642176 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109332438551860992,2461136.6350,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109332438551860992 20260406.1350 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115757262946945408,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115757262946945408 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8128-04.7311,2461136.6350,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.8128-04.7311 20260406.1350 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111015619053044352,2461136.6350,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111015619053044352 20260406.1350 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102785122 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6471-01.0142,2461136.6350,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6471-01.0142 20260406.1350 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115129785406375936,2461136.6350,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115129785406375936 20260406.1350 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.9547-01.7473,2461136.6350,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.9547-01.7473 20260406.1350 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3118345204080317440,2461136.6350,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3118345204080317440 20260406.1350 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071741.58-002045.0,2461136.6350,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071741.58-002045.0 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100477590376004224,2461136.6350,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100477590376004224 20260406.1350 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102806577,2461136.6350,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102806577 20260406.1350 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113913996125565440,2461136.6350,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260406.1350 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7378-03.3983,2461136.6350,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7378-03.3983 20260406.1350 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070654.13+021046.6,2461136.6350,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070654.13+021046.6 20260406.1350 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126155688009474560,2461136.6350,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126155688009474560 20260406.1350 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3377-03.4350,2461136.6350,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3377-03.4350 20260406.1350 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3118345204080317440,2461136.6350,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3118345204080317440 20260406.1350 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110870517879495168,2461136.6350,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110870517879495168 20260406.1350 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115523956026150144,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115523956026150144 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2427-02.0482,2461136.6350,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2427-02.0482 20260406.1350 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114962659637543808,2461136.6350,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114962659637543808 20260406.1350 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7472-00.7059,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7472-00.7059 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0704325-021741,2461136.6350,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0704325-021741 20260406.1350 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3155-00.0559,2461136.6350,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.3155-00.0559 20260406.1350 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108875037416696192,2461136.6350,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108875037416696192 20260406.1350 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5414-00.0643,2461136.6350,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5414-00.0643 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109541822495218944,2461136.6350,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109541822495218944 20260406.1350 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113219246514568576,2461136.6350,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260406.1350 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5890-05.1327,2461136.6350,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5890-05.1327 20260406.1350 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107553875417557888,2461136.6350,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107553875417557888 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 247,2461136.6350,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 247 20260406.1350 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108917372911018368,2461136.6350,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108917372911018368 20260406.1350 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119292502066292480,2461136.6350,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119292502066292480 20260406.1350 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108798488219749888,2461136.6350,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108798488219749888 20260406.1350 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059391727067990912,2461136.6350,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059391727067990912 20260406.1350 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101401729901835904,2461136.6350,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101401729901835904 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.1862-05.0049,2461136.6350,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J110.1862-05.0049 20260406.1350 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059023665547775232,2461136.6350,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059023665547775232 20260406.1350 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126750798678879360,2461136.6350,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126750798678879360 20260406.1350 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112746830169900544,2461136.6350,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112746830169900544 20260406.1350 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.6630+01.9547,2461136.6350,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.6630+01.9547 20260406.1350 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461136.6350,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260406.1350 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114707676020216448,2461136.6350,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114707676020216448 20260406.1350 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.1350 2461136.6350 13.36 07:06:37.26 +00:11:58.2
214.48694 3.46879 galactic Mon Second-epoch detections are separated by 3.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3114257834026347136 | 07:06:37.26 +00:11:58.2 (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) J-Ks=1.042+/-0.134 (M)
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 1.0rc89 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 3114257834026347136,2461136.6350,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3114257834026347136 20260406.1350 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114123143853389824,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114123143853389824 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126439671246457344,2461136.6350,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126439671246457344 20260406.1350 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3058297335039875456,2461136.6350,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3058297335039875456 20260406.1350 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0072-01.5341,2461136.6350,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0072-01.5341 20260406.1350 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113839096195943168,2461136.6350,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113839096195943168 20260406.1350 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3058809432579179264,2461136.6350,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3058809432579179264 20260406.1350 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8782+00.4793,2461136.6350,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J108.8782+00.4793 20260406.1350 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114747911273437952,2461136.6350,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114747911273437952 20260406.1350 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109710253931898240,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109710253931898240 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4148+01.7142,2461136.6350,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4148+01.7142 20260406.1350 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126334045110229760,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126334045110229760 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7299+01.6069,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7299+01.6069 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111221124647549312,2461136.6350,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111221124647549312 20260406.1350 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5037-03.5980,2461136.6350,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J109.5037-03.5980 20260406.1350 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9676+01.9141,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.9676+01.9141 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4678+01.8985,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.4678+01.8985 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052099353633714048,2461136.6350,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3052099353633714048 20260406.1350 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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
Mean magnitude and position on the discovery images:
2026 04 06.1350 2461136.6350 13.38 07:10:13.28 -01:12:05.9
216.14778 3.62819 galactic Mon Second-epoch detections are separated by 1.9" and 7.1 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 3109395419951972608 | 07:10:16.05 -01:11:48.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 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 3109395419951972608,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3109395419951972608 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9216-03.2652,2461136.6350,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.9216-03.2652 20260406.1350 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3060003742725747840,2461136.6350,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3060003742725747840 20260406.1350 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.9401-02.6616,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.9401-02.6616 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115597627604280832,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115597627604280832 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102696370481096320,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102696370481096320 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0819-02.9980,2461136.6350,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0819-02.9980 20260406.1350 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3554+02.5339,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.3554+02.5339 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114863772310812800,2461136.6350,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114863772310812800 20260406.1350 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108050304920710912,2461136.6350,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108050304920710912 20260406.1350 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0680+00.8355,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0680+00.8355 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1616-03.4790,2461136.6350,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1616-03.4790 20260406.1350 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.1103+02.0251,2461136.6350,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.1103+02.0251 20260406.1350 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9421-02.1958,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9421-02.1958 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107985536802150272,2461136.6350,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107985536802150272 20260406.1350 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3986+01.0587,2461136.6350,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3986+01.0587 20260406.1350 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113580985840495488,2461136.6350,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113580985840495488 20260406.1350 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7595+01.8088,2461136.6350,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.7595+01.8088 20260406.1350 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111869939586391936,2461136.6350,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111869939586391936 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108576073330848896,2461136.6350,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108576073330848896 20260406.1350 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.1919-01.4683,2461136.6350,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.1919-01.4683 20260406.1350 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 06.1350 2461136.6350 13.49 07:20:20.06 -00:44:21.3
216.90043 6.08617 galactic Mon Second-epoch detections are separated by 3.7" and 6.4 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 3110196650388708224 | 07:20:20.06 -00:44:21.3 (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) SpType: K5 (LAMOST DR5) J-Ks=0.700+/-0.035 (K)
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 1.0rc89 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 3110196650388708224,2461136.6350,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3110196650388708224 20260406.1350 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4081-03.5329,2461136.6350,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4081-03.5329 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8737+01.7832,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8737+01.7832 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059287239100606080,2461136.6350,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059287239100606080 20260406.1350 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127770183395674880,2461136.6350,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127770183395674880 20260406.1350 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3526-02.2087,2461136.6350,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3526-02.2087 20260406.1350 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059439349666232064,2461136.6350,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059439349666232064 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.1349+00.0658,2461136.6350,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.1349+00.0658 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112884548302958592,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112884548302958592 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7442-01.7579,2461136.6350,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7442-01.7579 20260406.1350 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114565839020994688,2461136.6350,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114565839020994688 20260406.1350 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.0348-02.6938,2461136.6350,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.0348-02.6938 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114789825855440512,2461136.6350,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114789825855440512 20260406.1350 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107976671995389184,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107976671995389184 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0835+01.6719,2461136.6350,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0835+01.6719 20260406.1350 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070541.48+024011.8,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070541.48+024011.8 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107637296560185088,2461136.6350,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107637296560185088 20260406.1350 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109759495740873216,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109759495740873216 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2862+00.7133,2461136.6350,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2862+00.7133 20260406.1350 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3164+00.4492,2461136.6350,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3164+00.4492 20260406.1350 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6636+02.0816,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6636+02.0816 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1271-02.9219,2461136.6350,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1271-02.9219 20260406.1350 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.6350,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.1350 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115136966591378816,2461136.6350,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115136966591378816 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5048+00.1592,2461136.6350,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.5048+00.1592 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.73CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127244578183449216,2461136.6350,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127244578183449216 20260406.1350 13.73CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0042+02.1543,2461136.6350,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0042+02.1543 20260406.1350 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059403375018906368,2461136.6350,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059403375018906368 20260406.1350 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2093-00.4486,2461136.6350,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2093-00.4486 20260406.1350 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110235103236646400,2461136.6350,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110235103236646400 20260406.1350 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.73CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071507.71+005721.0,2461136.6350,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071507.71+005721.0 20260406.1350 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5486+02.0516,2461136.6350,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5486+02.0516 20260406.1350 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7594+03.1305,2461136.6350,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.7594+03.1305 20260406.1350 13.79CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.82CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110966759505172352,2461136.6350,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110966759505172352 20260406.1350 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6350,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1350 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.4433-02.7092,2461136.6350,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.4433-02.7092 20260406.1350 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5244-01.2440,2461136.6350,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5244-01.2440 20260406.1350 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8703-03.7621,2461136.6350,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8703-03.7621 20260406.1350 13.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3099868941968800128,2461136.6350,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3099868941968800128 20260406.1350 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461136.6350,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Mon 20260406.1350 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0641591-011108,2461136.6350,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0641591-011108 20260406.1350 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J063207+0143.1,2461136.6350,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J063207+0143.1 20260406.1350 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0801 Mon,2461136.6350,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0801 Mon 20260406.1350 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0632358+003747,2461136.6350,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0632358+003747 20260406.1350 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Mon,2461136.6350,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Mon 20260406.1350 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461136.6350,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BM Mon 20260406.1350 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WY Mon,2461136.6350,9.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WY Mon 20260406.1350 9.89CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12582051,2461136.6350,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12582051 20260406.1350 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EG Mon,2461136.6350,9.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EG Mon 20260406.1350 9.51CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070529-0200.2,2461136.6350,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070529-0200.2 20260406.1350 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063753.27-055523.1,2461136.6350,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063753.27-055523.1 20260406.1350 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_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-Q1b1x1_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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DS Mon,2461136.6350,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DS Mon 20260406.1350 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461136.63538993 06.04.2026 03:14:47.690 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 118
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: 12 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): 39400
Objects passed selection criteria: 39371
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 36819
Average stars matched: 35145.2 (95.4541 %)
Memory usage VmPeak: 138564 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:01:56 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461136.63538993 06.04.2026 03:14:47.690 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 877
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 295 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): 252198
Objects passed selection criteria: 251594
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 233676
Average stars matched: 224398 (96.0293 %)
Memory usage VmPeak: 2005100 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 23:09:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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: 2461136.63468390
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# 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 06:51:32.738 -02:00:23.51
Angular distance between the image centers 0.0431 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:30.030 -02:00:20.79
Angular distance between the image centers 0.0544 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 06:51:32.738 -02:00:23.51
Second-epoch second image center 06:51:30.030 -02:00:20.79
Angular distance between the image centers 0.01130 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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.L85PqeIBYg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.Zh49i8IJqN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits &> /tmp/tmp.bykagwuqrf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits &> /tmp/tmp.0ldzxjO39l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_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 118 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.9 pix fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
2.9 pix fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.9 mag. fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
14.9 mag. fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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.L85PqeIBYg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.Zh49i8IJqN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
WARNING: 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.bykagwuqrf (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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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=3562, passed=37470
Got 37470 stars (including 33881 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat
util/solve_plate_with_UCAC5 got 37470 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 35766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 35767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 35766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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.0ldzxjO39l (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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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=3563, passed=37610
Got 37610 stars (including 34019 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat
util/solve_plate_with_UCAC5 got 37610 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 35674 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 35677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 35676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53518.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 3s
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Considering the candidate 52526_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52526_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:52.95 -02:53:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.010 3108144515015529728 107.97075632897 -02.88926494571 12.0010 11.2931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:37.34 -00:51:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.877 3109434035996804224 107.65552028332 -00.85265205601 12.3518 12.0002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52528_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52528_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:26.51 -00:43:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.878 3110938000404957440 107.86045949481 -00.72052171086 11.9417 11.5074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:28:39.21 -03:44:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:07.49 -01:28:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52536_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52536_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:51.25 +00:22:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 3.445 3113516389531142912 102.21376924338 +00.37265378636 11.0074 10.5246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52755_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 52755_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 52912_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52912_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:45.29 +01:49:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 3.772 3114146267953892224 104.68818322749 +01.81778760588 11.4391 10.9703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52931_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 52931_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:31.24 +01:05:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 4.996 3111748198735945984 109.38142228257 +01.09484165755 10.3371 8.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53055_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53055_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:03.68 +02:21:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53117_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53117_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:33.96 -00:06:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 0.414 3111219750258051840 107.14161387042 -00.10765030013 11.8466 11.6356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53129_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53129_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:31.32 +01:47:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53304_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53304_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:58.58 -02:46:09.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53352_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53352_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:26.52 -04:05:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.461 3107625343673873024 107.61035336955 -04.09863999365 11.9250 11.1617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53358_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53358_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:43.61 -02:58:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.514 3108666130203979904 105.68126598831 -02.97673526456 11.9522 11.3099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53359_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53359_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:39:59.14 -01:43:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 1.178 3106840670323834496 099.99645593540 -01.73188037468 11.3924 10.3738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53362_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53362_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:51.78 -03:43:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53365_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53365_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:09.63 -02:35:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.737 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53371_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53371_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:44:47.49 -05:17:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.648 3100694670902364416 101.19783487843 -05.29681766536 10.3253 8.7996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53388_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53388_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:09.14 -02:59:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.083 3108081847156522240 108.28809404572 -02.99188408101 11.8050 11.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53409_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53409_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:35:54.84 -03:57:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.233 3104828151726773888 098.97820694563 -03.96542848955 11.9193 11.4261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53420_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53420_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:45.30 +00:41:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.794 3114302329885570688 107.18869775869 +00.69614230443 11.9358 11.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53442_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53442_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:36:17.84 -05:48:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53445_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53445_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:35.41 -06:54:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53450_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 53450_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 53453_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53453_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:05.90 -01:21:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.438 3106351868685803136 102.77430949376 -01.36248533429 11.9159 11.5174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53462_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53462_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:36.57 -01:22:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.924 3107099119975852544 102.40225282149 -01.38158700736 11.9362 11.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53466_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53466_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 53467_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53467_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:08.70 -02:10:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.543 3109050723056765696 105.28607709374 -02.16803099465 10.6443 9.2354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53468_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53468_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:55.27 -04:15:42.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53473_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53473_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:36.16 -02:12:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53475_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53475_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:08.34 -02:29:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.526 3108979632757074560 104.28462469204 -02.48666262908 12.0874 11.9026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53481_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53481_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:02.74 -01:40:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 5.255 3112130038507187968 104.76201438618 -01.67860969947 11.9916 11.8110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:32:19.95 +00:04:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53486_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53486_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:44.23 -02:34:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53489_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53489_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:57.45 -03:41:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.896 3102646304044388352 104.23923477375 -03.69256330139 11.7371 10.9560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53495_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53495_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:07.17 -01:04:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.539 3112378974811857280 103.27975694621 -01.07747319334 11.6905 10.8183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53499_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53499_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:53.43 -04:09:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 2.271 3059574658313806720 108.22274210239 -04.15895316558 10.8218 9.3529 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53500_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53500_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:23:29.36 -02:44:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:06.79 -01:13:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 2.342 3112127873846137728 104.02800960912 -01.23330860926 11.8306 11.0479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:59.19 -05:10:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53518_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 53518_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 53520_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53520_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:01.90 -01:58:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.630 3106243184533303808 102.50792666588 -01.97042486853 12.1654 12.0227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53526_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53526_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:40.20 -03:16:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.243 3105807541711416448 102.91751408594 -03.27792843480 12.0078 11.8525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53530_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53530_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:43:57.72 -05:04:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:33.86 -03:01:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.619 3105850212204550144 102.89113279921 -03.02619808988 12.1065 11.9307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:54.30 -02:39:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.994 3106006347157749760 102.97621457366 -02.65496946936 12.0744 11.5523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:06.79 -01:21:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.292 3112286340957262976 103.52816984743 -01.35915272705 11.9522 11.5119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53539_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53539_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:07.13 -03:17:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.046 3102824905960778368 103.27958426428 -03.28844352308 11.9801 11.6215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53540_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53540_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:09.35 -03:05:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:43.79 -01:42:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53546_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53546_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:24.50 -02:50:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53548_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53548_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:01.57 -02:35:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.283 3105971880037872256 103.75633707660 -02.58618377942 11.9457 11.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53551_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53551_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:26:47.51 -02:31:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:50.98 -02:45:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.441 3105919275282129024 102.46229611178 -02.76586177128 11.9474 11.3776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53559_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53559_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:12.13 -01:48:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53560_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53560_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:02.67 -03:31:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53564_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53564_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:48.22 -04:51:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.597 3102075039031005056 103.20101982134 -04.85629740185 12.0596 11.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53565_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53565_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:54.58 -02:39:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.173 3106089046747361664 102.22766189689 -02.66193005359 12.0134 11.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:37.47 -02:54:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.158 3105716488402867584 101.65586277502 -02.90978906622 11.4636 10.2931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53567_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53567_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:19.13 -05:39:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53568_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53568_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:17.60 -02:07:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53569_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53569_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:59.18 -03:55:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.264 3107635239278364544 107.74647569970 -03.91972321891 12.2802 11.7686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:53.14 +01:22:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 4.151 3126065214517150080 102.72155493317 +01.36552187352 12.3588 11.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53572_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53572_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:22.96 -02:11:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.618 3109050031560612992 105.34531141623 -02.18446800678 11.9521 11.4806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53582_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53582_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:34.31 -01:20:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 5.432 3109527911102012288 105.89334737952 -01.33795777552 12.4184 12.1670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:23.86 -02:34:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:38.66 -01:08:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.177 3112331558372920960 103.66091366055 -01.13772716133 12.1235 11.9991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53599_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53599_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:48.87 -02:04:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53607_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53607_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:14.75 -02:44:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.073 3108734574801210240 105.31128390213 -02.73835436791 12.0107 11.5848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53611_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53611_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:49.70 -02:12:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.187 3108991693024899200 104.45688285094 -02.20724010665 12.1096 11.7006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53614_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53614_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:52.65 -00:38:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.122 3113159048254719744 103.21928317829 -00.63786247426 12.0765 11.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:22:07.36 -04:07:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.935 3116574440603444864 095.53040787951 -04.13080467050 11.8603 11.1153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:35:41.47 -04:40:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.543 3103911949303007232 098.92256185389 -04.68002939497 11.2832 10.0310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:58.05 -02:10:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.051 3106051182313984384 103.49187057041 -02.17906958237 11.8516 11.1276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53624_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53624_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:43:42.25 -03:17:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53626_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53626_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:45.63 -03:30:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:35.75 -04:56:39.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)
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Considering the candidate 53630_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53630_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:51.74 -02:29:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.932 3105931026312635776 102.71547327771 -02.49760872439 12.0741 11.6975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53632_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53632_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:42.56 +01:05:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.362 3114037313224363648 103.17728699802 +01.09762293268 12.0305 11.5866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:50.21 -05:33:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.265 3101894379828642944 102.95915856284 -05.56087713298 11.9962 11.6123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:28.37 +01:09:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.205 3125687600994081280 102.36823595003 +01.15494357196 12.1619 11.8897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53636_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53636_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:37:17.74 -04:58:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53637_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53637_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:32:41.30 +00:00:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:37.63 -03:25:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.443 3102798414602508800 103.15670783379 -03.41972905986 12.0065 11.5164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:53.36 -02:29:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53642_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53642_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:37.70 -06:49:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.786 3100799884723900032 103.65697364675 -06.83179397709 12.0515 11.6011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:50.39 -04:41:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.245 3059308267260336000 108.70995271486 -04.69945687364 11.8823 11.1128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53650_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53650_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:37:55.82 -01:31:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53651_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53651_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:15.93 -04:50:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.675 3101486357939094912 106.31642168106 -04.84271369638 11.9818 11.2815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:53.98 -03:02:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.478 3107984501716477184 106.47496166236 -03.03985352274 12.1878 12.0157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53654_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53654_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:20.53 -01:09:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53661_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53661_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:49.89 -02:57:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.461 3102933620172843264 103.45772980470 -02.95244580034 11.8589 11.1463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53663_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53663_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:45:42.11 +00:06:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.362 3113491336983178624 101.42545409096 +00.11364939674 11.9470 11.1019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53665_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53665_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:22:46.05 -04:29:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:09.38 -03:38:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.712 3105417661758290432 102.53901700476 -03.64244311062 11.8268 10.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53668_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53668_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:30.61 -00:45:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.033 3113186295525804672 102.37745406947 -00.76008801501 11.8936 11.1045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:09.42 -01:30:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.678 3112139521794982400 105.03975970277 -01.51490934545 12.2080 11.7641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53672_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53672_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:27.02 -02:05:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.726 3106240405695856640 102.36295632735 -02.09199322838 12.1173 11.8032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53678_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53678_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:50.05 -02:30:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.366 3106150722477720192 101.70886789962 -02.50965411492 11.8322 11.0362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53681_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53681_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:31.42 -02:06:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.958 3106202163304545664 101.88109323703 -02.10510799966 12.0383 11.5927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53686_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53686_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:58.88 -01:35:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.880 3107068677246859008 101.99551155933 -01.59949076215 12.3625 11.8757 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:45:46.05 -01:50:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.846 3106975356196809856 101.44182679957 -01.83717801208 12.1069 11.7910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53690_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53690_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:47.93 -02:24:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.939 3106122379993182208 102.44990402444 -02.41415379239 12.1563 11.9525 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53691_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53691_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:22:24.84 -01:42:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 3.387 3118286685148803584 095.60386669068 -01.70956087597 12.2053 11.8886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53694_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53694_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:37.47 -05:55:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.064 3058180095311536128 109.90613052400 -05.91943451038 12.3618 11.4331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:44:18.27 -01:40:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.268 3107008616425469568 101.07614640671 -01.66776842132 12.0246 11.5204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:12.93 -03:05:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:55.03 -05:39:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.058 3053138078580440064 107.72927321043 -05.65857123656 12.0165 11.3252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:14.00 -00:27:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.575 3112509026428065024 103.80743347266 -00.45561483097 12.8186 12.4804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53706_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53706_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:43.14 +00:08:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.896 3119554838670922112 100.67983280931 +00.13825526514 12.0665 11.5586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:43:35.95 -02:03:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:10.01 -01:44:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.240 3112073035703976704 103.79139523885 -01.73459395894 12.0587 11.6217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53721_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53721_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:28:59.53 -05:32:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53725_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53725_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:54.46 -06:02:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.376 3100386880667141120 101.72688877586 -06.03838166149 11.5473 10.3065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:45:33.20 -04:21:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.368 3105261114491085824 101.38808394531 -04.35119224614 11.8451 10.9959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53734_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 53734_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:31:54.38 -04:43:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.276 3104306841477505536 097.97640886925 -04.72366334936 11.5177 10.3998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:53.16 -06:53:23.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.71 -02:21:31.0
06:40:30.44 -01:04:41.8
06:26:05.11 -03:31:26.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# 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 06:51:32.738 -02:00:23.51
Angular distance between the image centers 0.0431 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:30.030 -02:00:20.79
Angular distance between the image centers 0.0544 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 06:51:32.738 -02:00:23.51
Second-epoch second image center 06:51:30.030 -02:00:20.79
Angular distance between the image centers 0.01130 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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.olpR1JNuaY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.ru4X88VHqO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits &> /tmp/tmp.c7yBySOyUQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits &> /tmp/tmp.lwGV090Y8B
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_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.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 816 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.8 pix fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
2.8 pix fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.1 mag. fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
14.1 mag. fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.olpR1JNuaY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.ru4X88VHqO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
WARNING: 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.c7yBySOyUQ (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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=34511, passed=212935
Got 212935 stars (including 178191 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat
util/solve_plate_with_UCAC5 got 212935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 207230 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 207229 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 207222 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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.lwGV090Y8B (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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=34748, passed=214011
Got 214011 stars (including 179020 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat
util/solve_plate_with_UCAC5 got 214011 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010457 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 205556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 205556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
WARNING: Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 205557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 939 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-13-46_20.00sec_-4.90C_LIGHTs_0032.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_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_2026-04-05_CI_Mon-02-Q1b1x1_221545_TTUQ1b1x1_10604_aCIfUNbA/wcs_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out265443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288281.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288312.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288374.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288472.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out290791.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out291333.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out293317.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out293671.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out295157.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out295330.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out295794.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out295864.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out08764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out230051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288562.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80449.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 458s
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: 225s
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Considering the candidate 288256_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288256_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:33:39.20 -06:17:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.418 3103106179078431104 098.41237831681 -06.28912610778 13.9214 13.4813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288278_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288278_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:39.89 -02:34:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.713 3102973756648649344 104.16547245953 -02.57433466669 14.6674 13.9687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288279_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288279_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:59.96 -06:49:21.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 288281_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288281_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:23.46 -01:45:10.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288298_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288298_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:56.10 -00:27:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.520 3112836749605360512 104.73364141525 -00.46255509166 14.2336 13.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288304_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288304_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288306_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288306_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288308_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288308_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:15.72 +00:05:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.499 3119541988128416896 100.06515014767 +00.09417658453 14.4011 13.7953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288312_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288312_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:59.59 -00:06:56.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 288320_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288320_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:49.96 -03:35:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.810 3107821018078608256 106.45768724526 -03.59019402716 14.5528 13.9722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288323_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288323_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:57.21 -02:28:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.802 3108793295594251648 106.48790490713 -02.48105391042 14.5732 13.8142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288329_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288329_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:33.86 +02:10:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.703 3115498431039332864 105.39099893226 +02.16720105851 14.4002 14.0382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288331_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288331_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:25.14 -00:51:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.601 3112572012122478976 105.35435761923 -00.86556119454 14.1848 13.5538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288336_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288336_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:50.01 -02:56:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.876 3060150321368252288 109.20795395772 -02.94073182240 14.2245 13.5071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:39:59.15 +00:54:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.761 3119847648062126464 099.99654025840 +00.91468433371 13.2693 11.8723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288339_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288339_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288345_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288345_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:59.75 +02:14:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.843 3115581444167631232 105.74880032372 +02.23716638684 14.4330 13.8658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288346_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288346_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:28.54 +01:59:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.357 3126176063334643456 102.86890551747 +01.99415086280 14.0851 13.6068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288349_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288349_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288350_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288350_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:29.88 -02:28:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.700 3108408470826506496 107.37515152719 -02.47940951283 14.1083 13.2369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288358_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288358_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288359_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288359_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288361_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288361_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:43.85 -02:06:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.228 3109052230584185216 105.43257930601 -02.10844515775 12.9740 11.4924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288374_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288374_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:02.90 -01:16:43.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288375_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288375_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:28.31 +03:01:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.865 3127842063967195392 103.61773770839 +03.02715183520 14.0948 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288383_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288383_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:35.97 +00:07:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.651 3111112547874786304 108.89966901416 +00.12247911678 14.0533 13.6115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288384_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288384_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288386_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288386_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:33.03 -01:18:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.855 3109170054426772992 105.38814548435 -01.30454717400 13.8072 12.7960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288390_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288390_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:27.97 +00:08:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.052 3111101071721707776 108.61640764718 +00.13405167302 13.9941 13.3505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:32.52 +01:13:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.480 3114427644151902848 108.13570439021 +01.21681422495 14.3290 13.9866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288396_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288396_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288397_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288397_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:21.16 -00:48:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.108 3110188614511257216 109.58836340239 -00.80415168852 14.4697 13.8440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288400_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288400_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288401_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288401_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288403_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288403_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288404_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288404_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:39.90 +01:10:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.335 3114427193177580160 108.16636845873 +01.17655047980 14.2983 13.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288405_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288405_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288411_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288411_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288413_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288413_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:53.38 -06:12:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.807 3100462781329477760 100.72226508825 -06.21026488446 13.9952 13.1871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288414_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288414_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288415_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288415_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288422_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:14.65 -05:48:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288423_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288423_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288426_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288426_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:23.49 +01:30:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.554 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288432_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288432_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:27.10 +01:35:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.075 3114511172674795264 107.36255922503 +01.58449736467 14.4418 13.7019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288446_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288446_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:49.20 +00:06:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.807 3111426252285597568 109.70508366275 +00.11378042853 13.9689 13.2747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288447_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288447_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:52.30 -05:18:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288451_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288451_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:29:31.57 +02:28:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.598 3124048439614249984 097.38157476050 +02.46605700743 14.0781 13.3972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288452_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288452_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:38.60 -03:28:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.522 3060013019854739456 108.66078206267 -03.47683759899 14.1066 13.5086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288453_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288453_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288456_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288456_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288461_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288461_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288462_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288462_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288470_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288470_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:40.44 +00:17:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.890 3110699887417878400 110.41885502054 +00.28280773611 14.4362 14.0322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288472_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288472_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:44.04 -02:38:44.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 288477_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288477_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:56.84 +02:23:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.549 3136003841858452224 109.98675025653 +02.39782322648 14.1344 13.6752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288482_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:21.60 +02:16:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:29:08.35 -06:31:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.168 3007195023871923072 097.28442425639 -06.52232081150 13.5384 12.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288491_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288491_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:20.17 -02:55:23.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 288493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288494_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288494_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288496_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288496_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:11.84 +00:06:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.148 3111242152807323776 107.29916214691 +00.09921903946 14.1644 13.3350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288497_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:11.59 +02:30:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.107 3126311956099234944 103.29819787042 +02.49941846084 13.9425 13.3871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288505_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288505_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288508_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288508_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:58.87 -05:05:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:05.76 -02:10:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288513_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288513_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288518_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:59.55 +02:11:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.756 3115580683954857216 105.74862171100 +02.18875778798 14.2908 13.4774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288520_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288520_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:41.54 -00:46:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.573 3109621025991824896 106.67343921714 -00.76995325981 14.2122 13.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:30.12 +00:31:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.246 3111362033933865344 107.87530299519 +00.52008705743 14.2172 13.4277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288528_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288528_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:42.60 -00:01:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.780 3111083720054378880 108.92746619878 -00.03013289273 13.7345 13.0456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:31:44.36 +02:37:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.709 3124065310244678144 097.93525832045 +02.62637870936 13.9133 13.1167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288531_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288531_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:50.34 +02:40:27.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288534_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288534_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:59.70 +00:17:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.050 3111268777308163328 107.49855490054 +00.28881453888 13.2434 11.9268 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:04.76 +01:22:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.287 3114494370763124352 107.77010562724 +01.36859081160 14.2598 13.9764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288538_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288538_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:10.26 +01:00:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.838 3125713821773344640 101.54272357930 +01.00410104796 14.2178 13.5838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288542_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288542_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288543_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288543_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:33.93 -03:20:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.109 3102627891523000960 105.14126619319 -03.33702339234 14.1723 13.6461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288546_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288546_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:26.71 +01:34:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288550_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288550_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:50.70 +01:14:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:24.32 +00:47:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.242 3111352962963851264 108.60090612424 +00.79717935405 14.0663 13.3705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288555_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288555_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288556_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288556_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:16.32 -03:43:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.798 3059847715151997312 110.06811764903 -03.73049289558 13.9876 13.2972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288557_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288557_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288559_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288559_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:45:47.24 -05:59:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.790 3100397669625141504 101.44666535656 -05.99579212220 13.4065 12.3822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288562_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288562_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288563_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288563_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288564_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288564_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:46.95 +01:14:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.130 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288565_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288565_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:37.01 -00:55:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.745 3110169854094015104 109.90436615869 -00.91961148235 14.0296 13.3653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288567_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288567_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:00.50 -02:27:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.921 3108382597944365184 107.75203705934 -02.45583826967 13.9392 13.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288568_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288568_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:51.83 +01:20:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.128 3115367211199527296 105.46601850960 +01.33474391831 14.0347 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288572_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288572_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:57.64 +02:49:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.535 3116003347394333696 106.49042808236 +02.82051758828 13.9886 13.5116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288577_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288577_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:42.20 +00:40:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:19.40 -01:01:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288587_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288587_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:36.44 -01:11:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.261 3110076395606547840 109.15198605998 -01.18433730177 13.8906 13.2007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:17.48 -04:28:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.726 3059647157360382208 109.82250830942 -04.47537882075 14.0986 13.8890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288593_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288593_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288594_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288594_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288600_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288600_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:29.53 +02:30:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.883 3115754509872056192 104.87304614867 +02.50886577454 13.8045 13.2690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288603_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288603_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:51.92 +01:08:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288608_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288608_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:47.36 +00:56:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288612_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288612_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:41.23 -00:09:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.514 3111043205623825792 109.17189007575 -00.15297107023 13.9845 13.6973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 288618_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288618_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288631_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288631_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:47.29 +00:55:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288632_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288632_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288633_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:54.40 -06:36:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288639_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288639_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:30.35 -04:15:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.557 3058928347334890752 110.37656508441 -04.26528772641 13.6573 12.9160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288642_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:45.52 +02:20:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288643_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288643_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288648_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288648_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:49.42 +00:45:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:51.45 +01:08:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:19.11 +02:39:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288655_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288655_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:39.76 +01:19:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288656_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288656_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288657_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288657_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288658_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288658_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:34.52 +01:34:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.196 3114874007212799872 107.89391146696 +01.58006011879 13.6108 13.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:20.67 -00:46:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.544 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288665_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288665_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:55.98 -04:42:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:28.87 +01:57:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 4.090 3126128578172313088 102.86979489983 +01.95042245078 13.6599 13.1801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288669_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288669_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:23.47 +01:06:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.891 3114460453403036288 107.34779969818 +01.11114139481 13.5564 13.0762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:28.18 +02:18:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288672_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:49.48 +02:13:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.236 3115664010613672832 104.95592961789 +02.21918834243 13.2142 12.3137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288674_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288674_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:51.84 +02:28:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288675_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288675_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:12.59 +00:51:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288678_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288678_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:35.58 +00:21:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.708 3111495349719112960 109.39824997400 +00.35741434228 13.5433 12.8735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288681_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288681_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288682_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288682_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288683_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:07.90 -03:36:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.245 3107706398298130688 107.53289140513 -03.61215099012 13.6312 13.0548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:30.17 +01:25:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288688_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288688_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:51.47 +02:28:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288689_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288689_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288690_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288690_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:29.21 +01:21:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.804 3114586076906068736 106.62167396384 +01.36430483885 13.5250 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288693_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288693_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 288695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:54.51 +01:48:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:10.38 -03:07:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.902 3060130942475902976 109.29324883491 -03.11950048425 13.3948 13.2747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288698_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:53.53 +02:27:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288699_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288699_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:39.78 +00:58:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:23:29.48 -02:32:14.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 288702_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288702_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:33.12 +01:14:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288703_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288703_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:43.57 +02:46:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.033 3127766919219874688 104.18143344956 +02.78191443907 13.3299 12.8376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288704_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288704_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:30.34 -06:31:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288709_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288709_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:13.36 +01:52:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:23.20 -00:49:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.220 3109432047432592384 107.84649073771 -00.82722994805 13.1589 12.4319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288712_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:31.84 -01:39:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.149 3106879595607559680 099.63337143534 -01.65868987318 11.4562 10.0112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:40.18 +00:33:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 4.072 3114284982518090752 107.41745075127 +00.56373048364 13.2043 12.4043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288714_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288714_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:16.96 +01:44:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288719_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288719_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288722_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288722_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288723_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288723_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:02.35 +01:07:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.793 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288724_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288724_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:54.59 +00:53:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.042 3113971690424905728 103.47724737496 +00.88351500760 12.1834 11.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288725_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288725_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:45.95 +02:36:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.101 3127768293610081152 103.94127315085 +02.61504769689 12.8271 12.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288726_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288726_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:36.16 -01:03:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.356 3109978607791727488 109.90068271934 -01.06720992550 13.1560 12.6554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288728_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288728_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:36.65 -01:40:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.851 3109456094950953344 106.15260396703 -01.66850726094 12.9200 12.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288729_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288729_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:11.12 -00:29:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.871 3112693400776779520 106.29629603399 -00.48935224730 12.8501 12.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288731_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:58.44 -02:15:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.733 3109178197686728960 106.74325949465 -02.25483112268 12.5852 11.7335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:05.12 -03:10:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 2.944 3108637100527185024 105.52093776583 -03.18124398695 12.9536 12.2166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288737_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288737_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288740_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288740_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:23.02 -01:05:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.674 3110103814678201216 108.84598631692 -01.09507289294 12.7058 12.5085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288743_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288743_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:18.40 -01:42:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 1.613 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288745_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288745_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:33.54 -06:41:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.292 3100770404068657024 104.38961396083 -06.69639988845 12.5350 12.1358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:26.81 -00:08:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.021 3110997305312695552 108.36182965332 -00.13554812095 12.3183 11.8240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288750_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288750_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 288751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288752_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288752_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:26.27 -02:17:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:09.99 -00:07:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288754_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 288754_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:52.26 -01:57:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289090_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289090_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:37.48 +00:27:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 1.010 3114280412673080576 107.15620925738 +00.46477827338 10.8261 9.9927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289340_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289340_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:31.31 +01:47:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289409_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289409_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:59.64 +01:36:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289581_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289581_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:51.78 -03:43:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289605_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289605_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:27.16 -03:20:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 3.008 3107881255000913152 106.36288380293 -03.34481404916 11.7246 10.8001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:09.13 -02:59:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.594 3108081847156522240 108.28809404572 -02.99188408101 11.8050 11.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:39.66 +00:25:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.500 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289705_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289705_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:30.43 -01:04:42.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 289836_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 289836_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 289864_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 289864_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:39.15 -04:12:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.673 3059689076241014272 109.91356328670 -04.21137790261 12.2923 11.8327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289940_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 289940_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290022_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290022_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:41.59 -00:33:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290103_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290103_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:26:56.32 +00:49:07.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290105_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290105_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290188_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290188_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:50.25 -05:11:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290200_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290200_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:21:53.74 +02:20:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290243_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290243_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:31.78 +00:27:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 2.407 3114280374012770048 107.13225247109 +00.45424085252 12.4613 11.6661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290279_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290279_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:16.70 -04:03:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 2.547 3107593870154767744 106.82014353931 -04.06254484292 12.5758 11.6556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290381_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290381_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:29.30 +01:00:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:37.45 +03:12:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 2.546 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290406_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290406_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:21:54.73 +02:22:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290425_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290425_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290501_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290501_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:13.18 -01:59:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.090 3108508526385840000 108.55471549568 -01.99146136572 12.9403 12.6341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290600_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290600_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:14.96 -01:12:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 2.326 3110107628608308992 108.56209306188 -01.21132212071 12.7166 11.8524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290615_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290615_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:22:45.44 -02:10:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:35.88 +00:49:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.416 3113827242086041984 104.89999945513 +00.83322365418 12.8202 11.8115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:52.48 -07:03:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:08.93 +00:16:36.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:15.90 +00:11:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.946 3111301595154963840 108.06597197083 +00.18423022844 12.8754 12.1576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 290784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:18.43 -05:24:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.721 3104187235226900352 096.82605277859 -05.40836792737 12.8062 12.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290791_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290791_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:19.95 -01:09:41.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)
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Considering the candidate 290794_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290794_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290834_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290834_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:22.38 -04:19:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.868 3059665436741207424 109.59307642061 -04.32519441867 12.9805 12.6967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.868#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290850_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 290850_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 290863_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290863_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:31.21 +00:46:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.979 3114351331172456192 106.87951415988 +00.76727923449 12.7081 11.6609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290924_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290924_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:18.38 -00:43:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.103 3110902055817540608 108.57636180658 -00.73251279606 13.0490 12.3529 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#
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Considering the candidate 290976_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 290976_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:52.65 +00:17:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.310 3111447039926977152 109.46937545194 +00.28408061663 13.0457 12.6048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291033_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291033_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:45:00.15 -00:03:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.970 3107483197430678400 101.25075565208 -00.05928951009 13.0563 12.7107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291047_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291047_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:39.62 -04:48:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291074_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291074_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:22.85 -04:08:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.586 3107533946769387392 107.34498467445 -04.14990516113 12.9877 12.2399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:38.96 -04:57:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.448 3101460553774510080 106.16235709519 -04.95151270632 13.1685 12.9202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291081_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291081_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:52.16 +01:55:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291131_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291131_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:55.48 -06:13:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291147_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291147_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291179_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291179_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291181_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291181_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:29:22.99 +02:43:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291216_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291216_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291253_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291253_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:52.15 +00:59:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291257_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291257_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:33:59.79 +01:45:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.317 3120911322481431936 098.49950014419 +01.75665840777 12.7992 11.9050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291274_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291274_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291280_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291280_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291313_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291313_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:54.21 +00:00:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 3.417 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291330_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291330_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291333_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291333_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:02.57 -03:29:52.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 291335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291342_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291342_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291366_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291366_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:26.45 -01:03:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.584 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291379_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291379_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291389_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291389_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:43.53 -00:29:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.004 3112692889681609088 106.18162536672 -00.49277504927 13.1660 12.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291417_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291417_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:51.53 -03:52:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.981 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291418_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291418_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:19.02 +02:16:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.264 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291435_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291435_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:28:24.19 +02:02:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291436_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291436_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:31:44.90 -05:21:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291456_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291456_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291466_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291466_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291470_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291470_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291476_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291476_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:52.42 -00:27:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 3.464 3109706135063598592 106.71842488065 -00.45571211931 13.1534 12.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291511_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:54.72 -02:07:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.262 3109185997347126144 106.97800092082 -02.12496158174 13.3108 13.0706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291517_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291517_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291542_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291542_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291545_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291545_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:17.46 -04:25:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291552_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291552_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:22.73 -06:08:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.516 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291576_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291576_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:34.22 -02:56:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.097 3108141083347828608 107.64208629129 -02.94531358274 13.3265 12.9641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:04.64 -05:12:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.297 3059182270101245184 108.26901293885 -05.20674695039 13.3733 12.8324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:32:16.68 -00:38:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291597_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291597_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:38.90 -02:48:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.964 3108710218049617536 105.16212073920 -02.81529430058 13.4054 13.1177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291616_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291617_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:25.26 -03:35:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:03.33 -02:29:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.188 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291651_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291651_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:05.15 +01:51:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.930 3114943486903722240 109.02124854035 +01.85665801526 13.5083 12.9759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291657_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291657_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:58.54 -00:56:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.544 3109605186152914432 106.99387176228 -00.94487186150 13.3450 12.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:13.55 +01:34:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.026 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291682_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291682_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:28.01 +01:29:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.660 3114638612946094336 106.36647147059 +01.49234473238 13.4661 12.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291715_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291715_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291790_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291790_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291795_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291795_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:51.38 -02:16:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.561 3108857002851931776 106.21398983457 -02.28187184212 13.3926 12.6907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291833_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291833_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291851_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291851_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:28.70 -02:27:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291857_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291857_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:48.86 +01:06:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.162 3113111528733238784 105.45369517809 +01.10034936016 13.6098 13.2914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291874_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291874_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 291885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 291896_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291896_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:39.06 -02:16:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291899_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291899_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:06.86 +02:39:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.508 3126327624139131904 103.27834999029 +02.66222062235 13.3598 12.4211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291905_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291905_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:55.10 -02:23:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 291993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:39.34 +01:03:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:22:26.69 -01:42:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.106 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292080_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292080_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:23.36 -01:36:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.572 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292106_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292106_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292108_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292108_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:44:11.55 +03:13:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.074 3127311480888772096 101.04831658328 +03.21883456912 13.4524 12.9837 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#
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Considering the candidate 292121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:14.76 -02:18:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.427 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292162_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292162_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:53.45 +02:12:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.073 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292163_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292163_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:37.32 -00:31:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.396 3112646160437322112 104.90516011811 -00.52192288748 13.4503 12.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292195_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292195_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292202_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292202_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292230_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292230_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292234_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292234_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:39.47 -00:16:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.449 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292237_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292237_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292263_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292263_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292264_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292264_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:20.59 -04:08:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.486 3107624690838876032 107.58557971057 -04.14945019378 13.5191 12.8389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292289_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292289_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:25.31 -02:06:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.532 3109746473400180224 109.85549204078 -02.10375818824 13.7381 13.2470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292298_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292298_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:57.96 +01:31:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.157 3111685732729870080 110.49156134520 +01.52740287703 13.5711 13.1752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292320_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292320_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:19.28 -04:08:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.203 3107624690838875520 107.58011994727 -04.14429608637 13.6473 13.2554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292387_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292387_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:59.63 -01:46:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.438 3109230802445716352 106.99827617880 -01.77454855490 13.6968 13.1802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292393_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292393_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292401_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292401_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292497_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292497_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292500_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292500_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:37.20 +02:26:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.741 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292504_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292507_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292507_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:39.79 -06:20:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:48.86 -06:01:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:00.09 -00:57:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.234 3109605181852110976 107.00017650752 -00.95349251268 13.5091 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292583_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292583_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:41.92 -06:20:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.897 3053036859096886656 107.42497549864 -06.33624383095 12.7148 10.9654 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:37.95 +01:08:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.924 3113112628244865152 105.40810060300 +01.13957680228 13.8333 13.5985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292614_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292614_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:38.53 -00:10:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.405 3112719548538664960 106.16109054830 -00.17571394208 13.5535 12.6595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292615_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292615_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:57.24 -00:05:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.612 3112885196837878016 104.98858288935 -00.08675063744 13.5793 12.7573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:50.30 -01:48:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.928 3109266055536999040 106.20982338393 -01.81483283230 13.7387 13.2803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292625_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292625_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:34.96 -04:56:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.951 3059249409029831296 109.39579258435 -04.93669882316 13.7381 13.0516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292628_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292628_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:06.31 +01:04:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.750 3113861189507185408 105.27604563182 +01.07345997565 13.3777 12.2598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:07.42 -01:40:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.012 3108576524307269760 108.28133940426 -01.67844425419 13.7420 13.2303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292645_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292645_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:47.38 +00:13:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.554 3113508143193552256 101.94725396759 +00.22585649620 13.6520 13.0798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292650_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292650_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:02.57 +02:09:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292654_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292654_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292660_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292660_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292721_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292721_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292722_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292722_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:57.15 +01:32:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.884 3111685737028265728 110.48816761873 +01.53364407573 13.7620 13.6454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292743_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292743_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:21.82 -00:32:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:43:53.39 +03:13:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.433 3127291139925000832 100.97237071891 +03.21786171975 13.5859 12.7087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292768_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292768_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:26.31 -05:18:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292772_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292772_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:29.74 -03:49:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.658 3107792709956047232 106.12420013624 -03.83445704157 13.8185 13.3765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292782_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292782_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292787_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292787_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292789_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292789_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:17.59 +02:31:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292833_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292833_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:08.10 +00:05:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292839_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292839_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292846_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292846_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292849_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292849_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:21.30 -02:02:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.738 3108460560189418752 107.58871498213 -02.03728762544 13.8016 13.2451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292865_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292865_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292878_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292878_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:39:32.24 +03:12:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.707 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:19.86 -07:10:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292907_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292907_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:48.01 -03:44:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292916_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292916_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292921_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292921_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292922_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292922_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292945_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292945_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292950_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292950_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292981_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292981_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292985_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 292985_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 292989_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 292989_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:04.42 -05:53:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293008_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293008_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:27.64 +00:09:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293013_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293013_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293029_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293029_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293034_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293034_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:25.93 -05:48:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 5.588 3100992264898211584 104.60868983330 -05.80991184590 14.0487 13.5345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293045_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293045_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293048_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293048_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293057_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293057_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293079_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293079_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:40.76 -07:13:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.371 3051750567927826688 106.92018204314 -07.22856050247 13.8622 13.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293082_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293082_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293099_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293099_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293100_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293100_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293101_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293101_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293106_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293106_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:52.85 -00:46:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293119_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293119_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:20.87 +01:51:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.869 3135914128582297344 110.33689970369 +01.85853796568 13.9525 13.4756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293126_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293126_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:54.37 +02:49:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293136_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293136_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293161_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293161_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:07.72 -05:35:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293166_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293166_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:27.00 -01:18:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293169_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293169_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293178_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293178_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293194_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293194_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:38.95 -01:16:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293195_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293195_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:04.13 +01:58:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.398 3126360472050420992 101.76704300021 +01.97593177349 13.9878 13.4960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293198_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293198_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:23.34 -00:09:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.269 3110294614303203840 109.59691543912 -00.15792757095 13.9002 13.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293201_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293201_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293206_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293206_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:21.03 -01:43:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293207_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293207_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293213_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293213_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:58.36 -06:07:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.225 3058263799935556352 109.49312850892 -06.12478401139 13.9696 13.2135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293222_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293222_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:33.34 +01:51:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.012 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293240_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293240_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293244_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293244_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293275_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293275_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293278_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293278_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:28.99 +01:07:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293280_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293280_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:05.42 -05:41:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.774 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293294_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293294_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293317_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293317_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:11.92 -02:28:31.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293322_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293322_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293328_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293328_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293338_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:39.44 -01:21:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.769 3109339619737041536 107.41478777276 -01.36419332163 13.8942 13.1712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293369_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293369_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:53.12 +01:49:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.117 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293376_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293376_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:47.01 +01:57:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293381_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293381_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293383_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293383_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:50.63 -03:01:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293387_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293387_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293400_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293400_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:44:50.38 +01:05:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.895 3125637783672257024 101.21022796390 +01.09398203346 14.0648 13.6219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293408_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293408_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:28:14.60 +01:53:14.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:47.47 -07:02:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293438_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293438_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293439_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293439_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:20.30 -05:15:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.443 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293451_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293451_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293474_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293474_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:01.82 +00:03:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.703 3111202810908018432 107.75743753981 +00.06395802188 13.6799 13.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293507_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293507_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:27.43 -01:23:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.378 3110089104408074368 108.61396742736 -01.40007490178 14.0204 13.6610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293514_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293517_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293517_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:32.50 +01:54:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293529_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293538_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293538_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293541_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293541_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293555_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293555_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:18.75 +01:08:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.356 3114463481358760448 107.32854114606 +01.13466947102 14.1091 13.5780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293560_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293560_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:51.18 -02:54:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.586 3108661530301553152 105.96319311778 -02.91418890016 13.9534 13.3027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293566_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293591_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293609_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293609_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:39:08.63 -03:48:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.768 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293620_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293620_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293625_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293625_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:15.21 +01:14:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.910 3125885414305835648 100.56374559839 +01.24197894342 13.9411 13.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293640_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:02:01.01 -00:33:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.405 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293645_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293645_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293647_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293649_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:35.76 +01:44:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:15.26 -00:32:57.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 293676_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293676_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293687_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293694_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293694_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293701_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293718_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293733_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293733_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:48.44 +02:30:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.074 3115039453652262016 108.45170061912 +02.51024491480 14.1789 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293753_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293781_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293781_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:27.43 +00:52:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293801_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293801_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293808_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293808_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293821_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293821_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:28.74 -06:01:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.130 3103166480420332032 099.61974936398 -06.02795289401 13.7856 12.9545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293826_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293826_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293827_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293827_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293829_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293829_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:25:45.33 -04:57:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293836_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293836_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:27.31 -05:52:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293859_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293859_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293883_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293883_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:52.42 +01:12:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293895_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293895_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:28:13.45 +01:53:01.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293900_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293900_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:16.30 -02:05:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.908 3108855903340435200 105.81770007262 -02.09964696229 14.0457 13.5449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293931_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293931_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:06.36 -01:59:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.006 3061725887170020864 110.52651101511 -01.99258502663 14.2307 13.6036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.006#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293934_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293934_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:40.09 -00:26:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.146 3112511367183611136 103.66730236160 -00.44919517720 13.9757 13.1957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293935_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293935_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:02.95 +02:18:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.791 3115584158586903424 105.76186017346 +02.31093887716 14.0901 13.5894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293948_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 293948_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 293954_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293954_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:06.92 +01:49:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.241 3115421087268758272 105.77929704766 +01.82442252696 14.0333 13.6803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293958_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293958_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:40.68 -05:15:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.247 3053401278483536128 106.41988000812 -05.26504640990 14.1538 13.7582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293959_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 293959_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:50.56 +02:53:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.569 3126481555767188608 101.96003040038 +02.88890140059 13.2729 11.9536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294003_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294003_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:35.41 -00:48:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.647 3112578162515589760 105.39724095265 -00.80783877429 14.1459 13.7567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294025_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294025_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:08.28 -01:43:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.719 3109786811733448832 110.28478090215 -01.72163301287 14.3217 14.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294030_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294030_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:24:05.08 +02:32:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294035_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294035_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294053_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294053_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:19.03 +03:02:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 4.573 3127835398178483712 103.82909987491 +03.03343876125 14.1871 13.7059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294068_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294068_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294073_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294073_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:12.90 +02:10:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294079_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294079_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294087_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294087_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:21.43 -00:32:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294115_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294115_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:42:19.66 +02:27:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.675 3126871195201213952 100.58243821561 +02.46094951773 13.4097 12.2445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294132_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294132_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:50.03 +00:09:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.538 3110689059801517312 110.45904011412 +00.15524258987 14.2131 13.7502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294135_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294135_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294147_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294147_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:08.24 -00:50:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294149_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294149_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:56.83 +01:49:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.652 3115415692790489728 105.98662008716 +01.81702803847 13.8554 13.0351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294169_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294169_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:14.33 -01:13:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.591 3110074505821408512 109.05984205440 -01.22298851226 14.1401 13.6720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294192_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294192_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294199_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294199_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:30:07.04 -02:39:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.776 3117217616247602048 097.52997534566 -02.66519300427 14.0065 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294214_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294214_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294216_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294216_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294226_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294226_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294232_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294232_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:03.39 -00:48:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.190 3109630955956555264 107.26411041079 -00.80830256355 13.9760 13.2107 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#
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Considering the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294242_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:52.69 -05:30:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.205 3101329677531128832 105.96948126070 -05.51097193635 13.4033 11.9481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294258_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294258_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294267_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294267_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:15.42 -02:19:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.276 3108285566046423424 108.56429063089 -02.32885347419 13.8739 13.2100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294268_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294268_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:58.32 -05:55:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294285_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294295_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294295_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294305_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294305_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:30:13.45 -05:57:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294310_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294310_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294312_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294312_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:38.66 -05:40:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294315_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294315_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294347_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294347_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:53.01 +02:16:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.659 3126232241506271744 103.47069199047 +02.27525024279 13.8274 12.8883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294352_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294352_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:57.27 +01:19:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.691 3114666925370467072 106.73881159656 +01.32597056953 14.2992 13.8046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294357_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294357_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294389_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294389_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294418_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294418_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:37.81 -03:05:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.628 3108124040917519872 107.90785244119 -03.09365330934 14.3096 13.8020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294421_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294421_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:26.74 +01:30:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294423_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294423_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:01:40.71 -06:28:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.567 3052844027942120704 105.42014323935 -06.48124281244 13.3943 11.6185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294435_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294435_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294439_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294439_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294454_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294454_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:11.11 -04:41:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.619 3059458625480286080 107.54607289320 -04.69148124863 14.2822 13.7450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294458_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294458_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294459_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294459_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:05.34 -01:23:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.712 3108602809506169728 108.27238188166 -01.38685283721 14.2787 13.7904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294473_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294473_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:00.74 -04:29:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.907 3101549270621282176 106.50250958880 -04.48726500273 14.3092 13.6969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294479_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294479_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:22.44 +01:18:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.088 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294482_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294482_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:52.45 -06:11:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.161 3052307333129613184 108.21869158369 -06.19603516741 12.9782 11.5663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:28.32 -05:22:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:24.40 -02:56:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.485 3108132768290673280 108.10144475205 -02.94555918877 14.2770 13.8047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294530_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294530_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:38.80 +00:36:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294578_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294578_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:26:29.79 +02:53:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294588_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294588_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:53:27.11 -00:36:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.927 3112409524919590528 103.36248731965 -00.60181293285 14.0759 13.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294604_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294604_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:10.55 -00:10:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.088 3109731561269564416 106.79359247673 -00.17885267927 14.4105 13.9138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294607_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294607_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:20.29 -00:32:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.105 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294635_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:37.42 +01:06:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294639_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294639_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 294641_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294641_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:35.74 -05:43:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.998 3053274422330454784 106.39896250904 -05.73294268524 14.2036 13.7409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294653_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294653_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:27.72 -01:34:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294656_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294656_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 294659_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294659_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294664_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294673_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294673_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:34.22 -02:33:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:45.61 -01:05:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.214 3109411637747856640 107.18988762013 -01.09938268298 14.2386 14.0433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294689_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294689_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294697_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294704_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294704_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294713_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294732_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294745_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294745_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:04.43 +02:53:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.520 3127827495438824576 103.76846723166 +02.88791128928 14.0788 13.1836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294750_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294750_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:57.42 -02:12:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.803 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294751_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:28.71 -01:01:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.971 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294765_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294765_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294766_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294766_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294767_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294767_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:09.89 +02:25:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294769_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294769_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294771_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294771_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294772_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294772_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:04.93 -02:24:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.152 3108412834513287936 107.27091703502 -02.40852093386 13.9961 13.1924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294773_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294773_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:47:09.30 +00:44:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.327 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294824_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294824_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294827_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294827_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294841_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294841_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:47.04 -05:52:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.711 3059074552323327616 108.19551815803 -05.87573455187 14.4696 13.9092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294848_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294848_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294851_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294851_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:57.71 -04:33:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294853_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294853_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294855_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294855_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294866_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294866_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:56:58.56 +00:23:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 5.064 3113693342185540992 104.24362456898 +00.39639448205 14.3425 13.7304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294871_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294871_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:48.46 +02:21:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.542 3115127242785262592 107.95181783413 +02.36243774016 14.2148 13.6586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294881_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294881_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294885_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294888_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294888_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:32:57.46 -02:23:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.907 3117243768307728000 098.23916846949 -02.38794555937 14.2908 12.8599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294901_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294901_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:35.24 +01:41:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.225 3114856041369812992 108.39690518346 +01.69802301952 14.2746 13.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294910_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294910_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294915_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294915_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294934_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294934_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294961_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294961_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:46.24 -04:14:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.543 3059716598390959232 109.44252754145 -04.23844785020 14.3995 13.6406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294966_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294966_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294968_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294968_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:44:20.91 +03:03:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.524 3127273650816868352 101.08693610723 +03.06251926918 14.1367 13.1163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294979_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294979_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294981_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294981_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:53.96 -00:43:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 294993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 294996_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 294996_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:16.09 -01:58:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.294 3109772552442329088 110.06730736101 -01.98023676963 14.1724 13.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295004_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295004_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295007_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295007_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:18.18 -02:07:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 4.816 3106051805090685696 103.57553630608 -02.12473732458 14.3576 13.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295009_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295009_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:51:51.82 -04:03:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.751 3102342980571017472 102.96630269222 -04.06398447247 14.2492 13.7474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295010_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295010_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295019_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295019_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 295030_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295030_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295031_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295031_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:17.66 -06:08:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.170 3053197662673353344 106.57364335646 -06.13618405435 13.8769 12.8596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295032_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295032_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:08.43 +00:58:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295055_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295055_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:25.88 -00:17:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.209 3110981465473380096 108.35766805675 -00.29126852768 14.5615 14.2022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295056_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295056_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295057_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295057_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295059_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295059_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:14.47 +00:26:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.136 3111136805849417088 109.06049235438 +00.43514316543 14.3578 13.8168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295067_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295067_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295069_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295069_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:13.01 -01:16:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.928 3110050690221476864 109.05428137357 -01.27936571809 14.2985 13.8244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295072_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295072_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295091_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295091_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:39.47 -05:23:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.440 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295099_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295099_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:37.43 -04:49:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.471 3059259442073403648 109.40551303626 -04.83077372288 13.8764 12.7591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295101_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295101_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:52.01 +01:51:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.034 3114852639755536640 108.71674078199 +01.86174097194 14.5626 14.0548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295105_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295105_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:04.03 -05:10:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.699 3101958735617958784 102.26698043601 -05.17603468037 14.3417 13.3664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295115_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295115_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:55.01 -05:55:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.560 3058171093060677120 110.22935140664 -05.92559192261 14.2618 13.4805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295118_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295118_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:18.34 +00:08:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.327 3111068876647108224 109.32611179926 +00.14271098473 14.4796 14.1904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295119_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295119_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:49:51.95 +00:49:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.183 3113659944517871104 102.46656884662 +00.83187008901 14.3851 13.8439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295123_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295123_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:06.27 -00:28:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.069 3112616817220941696 105.77637543341 -00.46842606859 14.2410 13.3658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295126_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295126_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:50.78 -01:45:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.672 3061838346592703872 110.46130091738 -01.75876978439 14.3741 13.7859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295127_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295127_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295143_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295143_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:31.77 -05:26:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295145_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295145_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:58.09 +02:05:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.628 3114788215246409088 106.74201411688 +02.09671466542 14.4155 13.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295146_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295146_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:39:18.06 -00:00:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.889 3119634037865932160 099.82526587339 -00.01402463254 14.4432 13.6701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295148_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295148_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:49.39 -01:36:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.961 3109847834630356992 109.70577252811 -01.60787785209 14.5971 14.0653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295149_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295149_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:15.17 +01:52:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.575 3114945101811423616 109.06375963615 +01.88242388147 14.4541 14.0144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295155_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295155_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295156_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295156_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:13.15 +00:50:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.698 3125567827244921728 101.55524044974 +00.83678768778 13.7948 12.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295157_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295157_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:28.00 -03:15:27.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 295166_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295166_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:14.02 +01:37:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.805 3111701989184527488 110.30833417745 +01.63172413329 14.4622 13.8136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295168_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295178_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295178_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295183_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295183_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295190_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295190_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295191_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295191_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295192_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295192_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295197_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295197_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:01.97 +02:55:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.986 3126526738822865536 103.00884024081 +02.91821182139 14.5084 13.6685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295200_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295200_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:50.34 -03:18:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.199 3108066728872333440 108.20957317665 -03.30848623413 14.4591 14.1870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295208_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295208_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295218_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295218_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:41.02 +03:03:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.162 3127097591516311424 100.42211117177 +03.05467666290 14.5145 13.4155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295226_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295226_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:46.88 -05:56:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.410 3053104272903239296 107.44589992980 -05.94152793165 14.1935 13.2741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295229_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295229_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:11.73 -05:42:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.601 3053310671852478464 107.04909467324 -05.70716089738 14.0992 13.3786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295241_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295241_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:24.49 +01:29:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.046 3114681837496746752 106.85213026201 +01.49026954613 14.3392 13.5511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295246_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295246_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:25.79 +01:52:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.733 3111956560486567680 109.60728421684 +01.87292226102 14.4800 14.1988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295254_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295254_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295271_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295271_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295272_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295272_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295275_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295275_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:48.84 +01:12:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.566 3111621072001178368 110.70379464731 +01.20098974083 14.2699 13.4170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295292_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295292_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:08.00 -00:54:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.839 3110134188686224896 109.28344042216 -00.90764436474 14.6052 14.0561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295296_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295296_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:18:51.91 -04:16:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.414 3059666604971496576 109.71617679170 -04.27355401424 14.4006 13.9225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295297_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295297_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:11.82 -02:38:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.509 3108355694269568768 107.54896724673 -02.63472009735 14.3810 14.0283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295313_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295313_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295325_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295325_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295327_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295327_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295330_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295330_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:53.59 -00:06:31.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 295332_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295332_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:26.43 -00:00:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.404 3111059977475066624 109.10994146627 -00.01784847256 14.5427 14.1391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295340_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295340_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:07.92 +00:04:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.572 3111097463949231744 108.53295337199 +00.06845340820 14.4902 14.2670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295355_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295355_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295372_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295372_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:56.58 -02:37:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.892 3061628339873347328 110.23650779964 -02.62382729351 14.5048 14.1048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295382_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295382_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295386_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295386_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:31.99 -01:32:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.750 3109884599548495488 110.38342280340 -01.54922469368 14.3952 13.7131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295392_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:04.39 -05:49:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.273 3058325544384670720 108.76887844313 -05.82290735052 14.2928 13.5412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295395_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295395_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:05.40 +00:51:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 5.360 3113605484332811648 103.02252679260 +00.85637243039 14.3468 13.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295406_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295406_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:46:20.88 +02:10:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.309 3126414657357026944 101.58709791842 +02.18050259777 14.1183 13.2209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295413_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295413_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295414_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295414_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:40.85 +02:13:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.135 3123946013232859776 096.92026605183 +02.21585268309 14.6313 14.0121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295417_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295417_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:03.02 -00:31:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.462 3110255886580485760 109.26278417022 -00.53316749974 14.3371 13.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295433_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295433_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295434_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:17.24 -01:49:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.936 3109789938469972736 109.82199501088 -01.83040186886 14.6043 14.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295441_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295441_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:50.73 -00:44:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.194 3110154151693617920 108.96153345098 -00.74143202661 14.4556 14.2633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295445_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295445_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:16:59.61 -01:25:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.282 3110030181758541312 109.24834244371 -01.42013320537 14.4440 13.9575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295450_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295450_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295452_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295452_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295454_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295454_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295465_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295465_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:04:35.10 -02:55:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.452 3108751518456730240 106.14659876532 -02.92747671806 14.4783 13.9795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295468_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295468_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295474_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295474_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:58.06 +02:35:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.949 3115187372326858112 107.24197816277 +02.59573875967 14.5487 13.9462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295476_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295476_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:04.18 +01:37:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295481_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295481_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:33.42 +02:43:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.327 3115954590926082944 106.88907883203 +02.71761943078 14.4306 13.7145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295483_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:46.51 -05:28:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295493_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295515_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295515_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:00.00 +01:56:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.776 3114902392656103424 107.99990533747 +01.94762214909 14.3530 13.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295527_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:20.04 +01:48:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.916 3115456202921062528 105.08373232209 +01.80654312181 14.5496 13.9285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295532_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:43.27 -01:49:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 295535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295535_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295540_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295540_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:34.30 +02:05:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.424 3114778800677883904 107.14263497990 +02.08825812307 14.5447 14.2668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295544_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295547_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295547_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:38:12.46 -04:02:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.747 3104065399894510976 099.55219263273 -04.04847604494 12.4601 10.8653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295554_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:27.13 +02:07:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.915 3114964618142610304 108.86303276636 +02.12785683820 14.5646 13.8699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295557_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295557_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295569_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295569_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:33.00 +02:15:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295570_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:46.17 +02:05:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.799 3114963381192015488 108.94228313476 +02.09086991176 14.5354 13.8132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295575_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295575_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:46.39 -00:35:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.986 3110392161600858112 110.44358245281 -00.59362381759 14.5562 13.9181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295576_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295576_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295577_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295577_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295578_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295578_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295585_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295586_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295590_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:13:12.64 -02:43:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.014 3108160634039606528 108.30275807212 -02.73436119346 14.4674 13.7650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295593_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295593_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295594_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295594_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:59.30 -02:29:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.903 3108381429714126592 107.74675809943 -02.48586767073 14.2019 13.4283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295595_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:24.11 -00:07:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.542 3111184187929791744 107.85033816158 -00.13283473894 14.3411 13.5573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295606_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:14.42 +01:38:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.809 3113952277172861952 104.80993462725 +01.63312300005 13.4969 12.0685 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295609_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295609_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295612_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295612_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295619_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:04.80 -03:43:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.183 3107621422360979328 106.76982168879 -03.72520651955 14.4877 13.9565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:50.98 -02:42:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 5.705 3108209905901244160 108.71191114651 -02.70952999906 14.4922 14.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295634_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295636_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295636_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295637_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295637_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295638_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295652_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:20:22.46 +00:21:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.990 3111460165347234432 110.09336709210 +00.36026980848 14.6450 14.1103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295659_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295659_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295666_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:39.94 -06:41:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.982 3052911136813625088 106.91620622114 -06.68669725775 14.5038 14.1616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295670_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295673_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295673_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295684_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295685_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295685_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295693_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295693_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295695_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295698_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295698_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295700_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295708_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295708_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295710_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295712_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295712_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295715_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295715_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:13.03 +01:31:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.910 3114676855335038464 107.05429841157 +01.52627513240 14.6476 14.1884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295717_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295717_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:42.91 +02:08:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.503 3115119168246936960 107.92858416975 +02.13449360873 14.6405 14.2384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295731_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295731_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295741_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295747_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:14.37 +00:19:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.638 3111495040481526016 109.30977713011 +00.32154863927 14.5964 14.0557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295749_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295749_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:34.02 -05:38:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.663 3059091457314434560 108.14151768990 -05.64985192415 14.1072 13.3046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295762_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295762_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295771_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295771_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:31.58 +02:41:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.776 3115211900883306240 107.38165054929 +02.69628619684 14.5842 14.0446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295773_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295773_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295775_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295775_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:25.40 -05:30:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.247 3053340942782660480 107.10548878502 -05.51391767214 14.5696 14.2967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295777_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295777_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:38.94 +00:06:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.020 3110687311753742976 110.41226806423 +00.10316143133 14.6336 14.0727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295778_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295778_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295781_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295781_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:24.14 -04:56:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.050 3102068068304979840 103.10112064737 -04.93798955510 14.5685 13.9898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295784_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:59.33 +01:35:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.618 3114502578441933440 107.74682409814 +01.59266012901 14.5715 14.0211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295787_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295787_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:23.60 -00:56:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.396 3110121922258856704 108.59817906051 -00.95029478632 14.5093 14.0765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295789_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295789_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:57.88 -00:52:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.968 3110884983328696064 107.99110653080 -00.87407211895 14.3560 13.9845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295790_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295790_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:41.12 -03:18:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.251 3107920253305420160 106.92097412871 -03.31215118348 14.6504 14.4151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295794_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295794_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:05:47.09 +02:22:14.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 295804_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295804_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295807_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295807_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295810_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295810_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295817_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:47.23 -05:01:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.113 3101986807523938688 102.69687570840 -05.02433398098 14.1141 13.0375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295821_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295821_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295823_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:22:08.45 -01:44:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.414 3061838995127651584 110.53533373568 -01.74446957439 14.5700 14.1399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295831_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295831_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295838_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295838_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:22.71 +00:52:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.514 3111400787420952192 108.59435183020 +00.87941299163 14.5488 14.0525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295843_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295843_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:20.76 +02:57:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.052 3115879995932377344 104.83668547342 +02.95508431458 14.5616 13.9521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295846_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295846_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:29.61 -01:29:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.967 3109864602182394880 109.37355349479 -01.48416585867 14.6850 14.4519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295864_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295864_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:45.67 +00:59:39.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 295867_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295867_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295869_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295869_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:15.70 +01:04:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295877_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295877_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 295882_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295882_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295884_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295884_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:01.05 -00:58:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.048 3109426927831923456 107.50440619152 -00.96959574901 14.6851 13.9026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295887_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295887_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295899_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295899_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:34.27 -01:45:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.198 3108563192728421376 107.64262776616 -01.76220649285 14.1788 13.4686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295901_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295901_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295905_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295905_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295907_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295907_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:36.37 -00:37:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.157 3110241700306339584 109.40120827384 -00.62739442917 14.5687 13.9475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295910_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295910_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:07.97 -02:23:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 3.856 3108413036369923072 107.28310332058 -02.38526041060 14.1226 13.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295915_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295915_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:24.79 -00:17:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.696 3109712659115220864 107.10346404505 -00.29265099079 14.4327 14.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295916_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295916_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:21:52.99 +00:01:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.839 3110639105040826752 110.47087902007 +00.03121623899 14.5918 14.1607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295919_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295919_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:14:42.25 -02:20:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295938_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295938_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:48:22.44 +01:01:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.049 3125668015943753984 102.09377189004 +01.01817011609 14.6347 14.0013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295944_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295944_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:33.84 +02:15:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.035 3115685382374762624 105.14085893802 +02.25199924638 14.6187 13.7152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295955_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295955_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:15:58.85 -02:16:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.981 3108294843176808576 108.99521570166 -02.27030020588 14.2973 13.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295960_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295960_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:15.40 +02:32:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.292 3115150779205995776 107.81444204717 +02.53191718088 14.7604 14.3422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295964_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295964_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:08:56.57 -00:19:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.274 3109665070877533952 107.23566746406 -00.32260317632 14.4466 14.0289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295973_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295973_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 295978_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295978_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:43.35 -02:39:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.624 3108173999977847680 108.18079931759 -02.65309653807 14.2970 13.9347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295982_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295982_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:38.10 +01:11:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.828 3114461213615946752 107.40898319460 +01.18470697774 14.7612 14.4368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295983_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295983_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295985_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295985_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:17:07.60 +00:12:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.088 3111071522346947968 109.28115885750 +00.20558640003 14.6812 14.0096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295988_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295988_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295995_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 295995_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 295997_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295997_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:41:11.07 +01:42:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.695 3126663524942570240 100.29656868349 +01.70354650098 14.6764 13.9899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295999_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 295999_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:32.38 +02:33:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 5.140 3115570479110574464 106.63489684324 +02.55376674315 14.6769 14.1366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296003_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296003_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:42.18 -00:35:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.316 3112599602992583168 105.92611366219 -00.58925302145 14.4325 13.6354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296004_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296004_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:59:38.51 -05:11:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.167 3101581908065366016 104.91021577897 -05.18993751339 13.6287 12.3354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296023_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296023_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:35:44.79 +01:10:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.982 3120656480601631104 098.93679045394 +01.17825266796 14.1636 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296027_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296027_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:10:48.23 -04:17:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.608 3059487487659940480 107.70097586290 -04.28944653727 14.3064 13.5222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296032_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296032_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:54:13.39 +02:59:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.252 3127841582930879232 103.55560175174 +02.98961188694 14.6187 14.0956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296045_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296045_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:27:49.84 +01:08:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.001 3123433297216721664 096.95764070686 +01.14005580527 14.2095 13.2377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296061_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 296061_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 296065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296065_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:52.82 -05:47:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.114 3100970034147527808 104.46977427493 -05.79430588640 14.1401 13.1482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296066_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 296066_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 296067_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 296067_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 296068_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 296068_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 296069_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296069_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:00:08.46 +02:10:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.870 3115686133990438272 105.03505900702 +02.18079468882 14.7151 13.8510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 296075_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 296091_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296091_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:55:45.96 +00:37:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 5.646 3113759549101578752 103.94190592996 +00.62784613966 14.5783 13.9309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296092_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296092_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:27.83 +02:07:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.353 3126187505126732672 102.61583098498 +02.11665875632 14.3199 13.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296109_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296109_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:11:17.83 -04:51:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.008 3059404989926960896 107.82440417551 -04.86285565371 14.2314 13.6329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296121_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:38.92 -03:39:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.650 3059862352400573184 109.91228997904 -03.66553424691 14.5440 14.0574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296127_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296127_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:07:55.00 -02:17:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.592 3109174929210280320 106.97938927799 -02.28619493009 14.7216 13.9160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296131_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296131_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:06:00.40 -01:01:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.199 3109520832995501184 106.50138230279 -01.02895292775 14.6394 14.0369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296201_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296201_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:58:44.94 -02:12:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.344 3109002752559773184 104.68691826078 -02.21644699691 14.8326 14.2518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 296335_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:57:31.67 -07:11:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.536 3052686870800815616 104.38207393811 -07.19372560730 13.9558 12.6836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 265443_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 265443_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:52:00.49 +00:12:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.268 3113357819339125504 103.00115885910 +00.20192758615 11.7103 10.0166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 08764_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 08764_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 237671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 237671_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:40:08.81 +01:22:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.930 3126632974834859392 100.03692742394 +01.37171623584 12.6357 11.1251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 154583_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 154583_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 230051_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 230051_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:50:00.72 +01:46:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.967 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 67537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 67537_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 06:21:55.08 -04:30:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200336_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 200336_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 121122_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:09:13.70 -02:21:31.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 31629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 31629_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:12:52.13 -05:20:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57802_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 57802_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 47993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 47993_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:19:38.70 -02:00:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033 did not pass the final checks
**** FOUND 07:03:53.15 -06:53:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80449_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 80449_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 131156_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 131156_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 31804_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 31804_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
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Considering the candidate 47889_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
Preparing report for the candidate 47889_fd_Mon-02-Q1b1x1_2026-04-05_22-14-47_20.00sec_-4.90C_LIGHTs_0033
make_report_in_HTML.sh Phase 2 (HTML assembly): 21s
make_report_in_HTML.sh TOTAL: 704s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.71 -02:21:31.0
06:40:30.44 -01:04:41.8
06:26:05.11 -03:31:26.5
06:41:48.23 -06:55:07.2
07:05:28.64 -02:00:08.1
06:41:59.22 -01:11:10.0
07:08:45.27 +00:41:48.2
06:32:36.12 +00:38:18.8
06:32:07.39 +01:43:00.1
07:17:31.21 +01:05:39.1
07:05:27.95 +00:36:30.6
07:08:51.33 -02:26:19.9
06:57:55.39 -00:13:52.7
07:11:32.32 +01:26:33.4
07:17:45.13 -00:17:16.0
07:14:06.90 -04:20:52.6
07:13:12.01 +00:38:43.6
07:09:04.05 -01:41:57.0
07:07:34.54 -03:27:34.7
07:01:58.09 -02:16:28.4
06:54:14.52 +03:03:39.4
07:13:26.54 +00:56:15.8
07:14:18.34 -04:09:01.6
07:06:56.23 +00:23:23.9
06:59:25.19 -01:21:53.4
07:08:52.74 -04:21:47.6
06:46:26.52 +00:59:02.8
07:11:47.40 +01:41:59.3
07:05:45.60 -02:32:43.4
06:27:32.84 -01:10:22.5
07:17:25.66 -04:17:48.9
06:55:54.31 +02:54:13.9
07:17:32.78 +01:33:25.8
07:19:27.98 -02:42:29.5
06:49:31.00 +01:58:04.3
07:15:27.30 -02:29:46.1
06:56:57.91 +00:29:34.9
06:55:37.51 +02:46:14.4
07:11:19.76 -03:51:44.5
07:04:32.14 +00:11:23.7
07:09:20.41 +00:20:20.3
06:57:22.88 +02:20:21.3
06:50:58.57 +01:35:34.5
07:16:40.42 -01:23:38.8
07:16:08.79 +00:47:13.0
07:06:18.03 +01:07:23.6
06:43:03.07 -03:21:50.2
06:28:19.58 -04:08:29.6
07:21:21.93 -00:51:52.0
07:22:07.41 -02:10:22.0
07:15:05.82 +02:37:23.0
07:08:31.17 -00:56:08.8
07:02:33.02 +02:20:26.1
07:10:48.74 -00:38:30.1
07:21:31.52 -01:38:19.3
07:20:31.64 -06:57:28.9
06:43:46.45 -05:42:08.3
07:19:44.76 -03:04:57.8
07:19:24.39 -00:41:30.7
07:09:37.99 +02:07:35.5
07:03:23.58 -00:39:16.9
07:16:58.56 +00:50:26.6
06:30:15.22 +02:16:00.3
07:21:59.34 -02:01:00.5
06:40:48.78 -00:33:38.5
07:22:32.66 -01:44:04.6
07:09:40.94 -04:22:45.1
06:54:23.70 -04:11:37.9
06:45:28.99 +02:24:20.5
07:08:24.79 +02:46:17.7
07:12:48.84 +01:20:08.9
07:08:57.65 -03:05:11.0
06:51:10.45 +01:06:00.5
07:22:33.94 -00:33:48.1
06:54:45.16 +02:52:16.0
07:07:09.33 -01:15:16.3
07:19:26.37 -01:55:44.5
06:46:13.86 +00:50:45.3
07:04:02.03 +02:51:32.4
07:06:31.68 +02:11:36.3
07:13:29.26 -04:08:39.0
07:11:19.66 -02:24:42.3
07:20:20.02 -01:34:22.0
07:03:38.84 -02:31:45.3
07:10:38.42 -00:26:09.2
07:15:07.42 -00:40:05.2
07:09:45.49 -03:50:37.7
07:07:26.07 -02:04:10.2
07:07:25.92 -01:50:45.1
07:14:00.43 -01:15:31.0
07:04:10.66 -03:14:37.6
07:13:41.67 -03:55:39.1
06:44:27.29 +02:30:55.7
07:00:37.09 +02:24:01.4
07:13:34.27 -04:04:38.4
07:14:59.16 -01:45:25.0
07:18:23.24 +01:03:42.2
07:11:08.09 +00:18:35.8
07:12:47.77 -02:27:16.8
07:17:28.74 -01:41:40.3
07:18:29.75 -00:11:36.0
07:16:55.49 -04:32:30.0
06:56:45.63 +00:46:09.1
06:56:45.10 +00:46:34.7
07:17:15.35 -02:36:55.8
07:13:39.24 +00:17:18.6
07:05:46.99 +00:13:15.3
07:13:03.13 -04:47:14.1
07:07:11.25 -02:58:19.6
07:10:57.64 +01:38:35.0
07:21:06.40 -03:14:57.8
07:15:46.86 -01:58:00.5
07:09:56.39 -04:34:53.5
06:56:02.79 +02:23:22.8
07:14:45.36 -06:00:15.5
07:12:56.17 +02:36:39.4
06:43:50.32 +01:35:50.8
07:00:51.99 +00:12:01.1
07:20:03.58 -01:48:50.5
07:08:11.40 -02:49:43.0
07:15:25.90 -01:11:23.0
07:10:02.55 -02:31:59.1
07:18:12.82 -01:43:03.6
07:01:10.19 +00:00:19.9
06:56:48.94 +00:46:32.8
07:11:37.83 +01:05:41.3
07:04:16.64 -03:01:37.2
07:11:45.29 -05:40:08.5
06:58:35.34 -04:20:25.8
07:05:20.36 +02:45:54.9
07:14:45.29 -01:22:49.3
06:58:50.12 -04:41:10.2
07:04:34.56 -05:56:28.1
06:49:52.97 +02:30:14.8
07:18:29.79 +00:52:08.9
07:19:08.27 -02:01:49.6
07:15:10.04 +00:21:59.8
06:37:16.15 +03:08:57.2
07:15:39.53 -00:49:28.3
07:10:42.55 -01:49:35.9
06:22:43.46 -02:10:03.9
07:17:41.20 +00:07:00.0
07:10:41.81 -02:46:24.7
07:08:10.19 -03:43:12.7
07:14:06.75 +01:28:20.5
07:04:33.73 -04:28:38.5
06:45:39.05 +02:45:24.8
06:36:32.32 -03:35:55.2
07:16:50.04 -03:31:10.0
07:19:06.80 -02:29:52.0
07:21:16.78 -03:12:16.2
06:49:16.17 -06:30:09.0
07:19:50.40 -02:35:19.8
07:05:20.53 +02:02:06.0
07:07:01.92 +00:40:29.5
06:45:09.47 +02:51:11.5
06:54:39.42 +02:38:00.9
07:09:28.97 -06:44:34.8
07:05:49.20 +02:34:31.7
07:10:49.21 -05:23:04.9
07:16:08.09 -03:04:46.8
06:35:10.41 -00:43:19.3
06:49:07.32 -01:40:17.6
07:11:20.02 +01:36:58.4
07:09:24.18 -01:33:15.7
06:58:57.63 +02:32:41.3
07:02:37.62 -01:54:05.5
07:15:16.33 -04:43:31.4
07:16:20.97 -00:19:45.3
06:45:33.70 -00:26:15.8
06:58:35.93 -01:00:30.4
07:12:48.06 +02:19:47.3
07:05:38.60 +01:26:03.2
07:15:49.13 -01:44:51.8
06:24:33.45 -01:26:13.6
07:17:42.14 -00:21:03.7
06:42:30.91 -06:04:21.1
06:46:10.28 -03:13:59.7
07:08:44.77 -01:27:54.2
06:57:35.55 +01:13:54.5
07:10:59.09 -03:24:27.9
07:06:54.08 +02:10:49.3
06:48:33.24 +01:48:58.0
07:01:18.50 -03:25:51.2
06:24:34.49 -01:26:23.8
07:13:40.78 -01:01:26.1
07:04:13.55 +01:59:53.3
07:08:58.12 -02:02:47.5
06:56:39.71 +00:24:11.4
07:15:35.43 +02:02:01.7
07:07:02.56 -00:42:25.6
07:04:32.63 -02:17:38.7
07:17:17.77 -00:03:13.1
07:03:45.85 -02:09:34.0
07:10:10.01 -00:03:44.9
07:03:46.90 -01:04:51.3
06:50:41.49 -00:31:45.0
07:02:23.39 -05:08:56.1
07:08:52.69 -03:55:19.2
07:17:36.38 +00:20:10.6
06:58:22.52 -02:33:47.8
06:32:37.47 -00:21:32.4
07:07:03.67 -02:21:52.0
07:01:49.42 -05:35:31.2
07:11:30.81 -04:56:27.0
06:34:16.11 -05:20:19.0
06:53:13.84 -04:35:47.4
07:17:12.67 +02:26:39.2
07:01:28.02 -05:15:03.7
07:20:44.53 -05:00:15.3
07:21:46.89 -04:08:39.8
06:38:49.79 +02:05:40.6
07:05:52.53 -00:00:59.4
06:38:39.42 +01:56:42.6
06:58:33.92 -01:38:09.5
07:10:03.22 +01:44:56.9
07:06:37.26 +00:11:58.2
06:48:56.93 -03:30:57.1
06:55:44.95 +01:32:28.0
06:46:16.57 +02:25:30.3
07:14:25.25 -06:11:44.0
07:08:01.10 -01:31:58.2
06:58:04.61 +00:51:04.1
07:21:22.39 -05:02:55.9
07:15:31.16 +00:28:43.2
07:07:06.62 +01:52:36.0
07:07:59.65 -00:24:51.6
07:09:36.21 +01:42:30.9
06:53:20.62 +02:43:17.5
07:18:54.14 +01:36:32.4
07:08:49.10 -00:04:32.4
07:18:00.41 -03:35:48.4
07:11:50.14 +01:30:57.6
07:11:49.96 +01:54:46.1
07:00:33.69 -00:05:51.2
07:13:50.70 +01:53:52.8
07:11:23.67 -07:04:29.5
07:16:03.21 +01:36:13.2
07:10:13.28 -01:12:05.9
07:11:38.89 -03:15:42.0
07:13:41.27 -03:39:08.7
07:15:45.85 -02:39:23.4
07:03:00.75 +02:24:11.0
06:58:47.95 -03:05:31.3
07:00:20.05 -02:59:45.0
07:21:26.49 -04:48:08.0
06:47:44.80 +00:19:24.4
07:17:25.27 +02:31:58.2
07:14:29.95 +01:49:08.2
07:13:14.78 -03:26:46.1
07:20:05.61 -00:29:44.4
06:52:19.01 +00:50:19.6
07:21:28.67 -04:04:57.4
07:08:41.07 -03:29:16.1
07:20:29.07 +02:01:14.6
06:55:50.64 -02:12:28.4
07:06:50.68 -03:05:03.4
07:16:41.81 +02:29:08.8
06:57:36.17 +01:03:44.4
07:21:23.98 -00:37:27.2
06:52:34.69 +00:32:34.8
07:14:59.81 +01:48:09.3
07:16:03.06 -00:40:39.8
07:17:35.03 +01:29:52.9
06:52:02.71 +01:24:02.0
07:14:33.99 -05:29:12.2
07:12:55.88 -01:41:31.2
07:16:46.06 -01:27:55.3
07:20:20.06 -00:44:21.3
07:09:36.61 -03:32:25.0
06:51:24.46 +01:46:42.6
07:05:39.86 +02:28:20.2
07:20:37.02 -05:27:07.1
07:14:12.32 -04:54:52.4
07:10:20.63 -00:55:59.4
07:14:23.75 -00:00:49.6
07:01:34.41 +01:46:03.5
06:55:56.27 +02:39:57.3
07:20:05.65 +01:09:50.0
06:30:11.26 +01:52:30.9
07:05:25.56 -02:12:22.9
07:09:37.42 -04:39:36.0
07:12:32.05 +00:04:09.4
07:03:51.50 +02:00:05.0
06:59:46.42 -00:07:54.4
07:10:55.03 -01:45:30.6
07:06:43.05 +01:06:56.7
07:12:07.31 -02:41:42.0
07:08:40.99 -00:53:47.0
07:06:31.61 +02:05:37.7
07:18:14.36 +00:02:43.8
07:05:56.42 -03:14:54.0
07:00:01.63 -04:09:57.6
07:19:23.66 +00:34:09.9
07:04:19.74 +01:39:45.5
06:54:25.05 -00:23:50.1
07:20:55.56 +00:36:26.3
07:12:26.80 +02:04:47.0
07:12:20.26 +01:25:29.4
07:21:03.32 +00:12:22.6
07:05:41.30 +02:40:15.0
07:08:39.92 -02:15:36.2
07:11:29.22 -03:50:43.6
07:13:14.15 -01:39:24.3
07:17:41.55 -02:02:57.4
07:14:46.42 -01:18:37.0
07:13:29.25 -00:50:57.8
07:09:08.35 +00:42:47.5
07:09:13.17 +00:26:49.8
06:42:39.82 +02:05:23.9
07:00:30.73 -02:55:25.7
06:59:37.53 -02:43:47.3
07:11:10.01 +02:18:12.0
07:18:00.81 +00:09:40.9
07:16:14.82 -00:14:34.3
07:13:34.72 -00:26:21.7
06:45:21.84 +02:57:34.8
07:07:59.09 +02:08:45.2
07:12:22.74 -04:42:42.9
07:12:48.01 -00:27:16.3
07:09:12.86 -00:34:11.6
07:17:16.56 -00:42:24.4
07:12:17.34 -01:40:18.5
07:10:33.95 -00:34:04.4
07:14:05.46 +00:33:06.9
07:22:28.38 +00:11:02.8
07:15:08.46 +00:57:32.7
07:13:04.11 -01:16:35.5
07:12:53.04 -00:10:58.7
07:09:52.27 +00:44:50.4
07:10:10.10 +02:03:17.9
07:16:17.04 +01:00:36.5
06:59:22.85 +02:14:38.5
06:47:02.60 +03:07:54.3
07:11:43.64 +02:18:05.1
06:55:40.98 +02:55:19.8
07:11:39.57 -00:20:22.1
07:02:45.30 -04:03:44.7
07:17:46.83 -02:42:16.0
07:02:06.97 -01:14:09.2
07:03:30.37 -03:45:39.9
07:09:11.19 -05:50:47.6
06:37:53.09 -05:55:16.3
06:44:47.48 -05:17:45.6
06:51:26.28 -05:15:26.0
06:45:42.35 -04:56:34.2
06:27:01.32 -04:35:40.9
06:52:06.22 -04:01:52.3
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:09:13.71 -02:21:31.0
06:40:30.44 -01:04:41.8
06:26:05.11 -03:31:26.5
07:05:27.95 +00:36:30.6
07:08:51.33 -02:26:19.9
06:57:55.39 -00:13:52.7
07:11:32.32 +01:26:33.4
07:17:45.13 -00:17:16.0
07:14:06.90 -04:20:52.6
07:13:12.01 +00:38:43.6
07:09:04.05 -01:41:57.0
07:07:34.54 -03:27:34.7
07:01:58.09 -02:16:28.4
06:54:14.52 +03:03:39.4
07:13:26.54 +00:56:15.8
07:14:18.34 -04:09:01.6
07:06:56.23 +00:23:23.9
06:59:25.19 -01:21:53.4
07:08:52.74 -04:21:47.6
06:46:26.52 +00:59:02.8
07:11:47.40 +01:41:59.3
07:05:45.60 -02:32:43.4
06:27:32.84 -01:10:22.5
07:17:25.66 -04:17:48.9
06:55:54.31 +02:54:13.9
07:17:32.78 +01:33:25.8
07:19:27.98 -02:42:29.5
06:49:31.00 +01:58:04.3
07:15:27.30 -02:29:46.1
06:56:57.91 +00:29:34.9
06:55:37.51 +02:46:14.4
07:11:19.76 -03:51:44.5
07:04:32.14 +00:11:23.7
07:09:20.41 +00:20:20.3
06:57:22.88 +02:20:21.3
06:50:58.57 +01:35:34.5
07:16:40.42 -01:23:38.8
07:16:08.79 +00:47:13.0
07:06:18.03 +01:07:23.6
06:43:03.07 -03:21:50.2
06:28:19.58 -04:08:29.6
07:21:21.93 -00:51:52.0
07:22:07.41 -02:10:22.0
07:15:05.82 +02:37:23.0
07:08:31.17 -00:56:08.8
07:02:33.02 +02:20:26.1
07:10:48.74 -00:38:30.1
07:21:31.52 -01:38:19.3
07:20:31.64 -06:57:28.9
06:43:46.45 -05:42:08.3
07:19:44.76 -03:04:57.8
07:19:24.39 -00:41:30.7
07:09:37.99 +02:07:35.5
07:03:23.58 -00:39:16.9
07:16:58.56 +00:50:26.6
06:30:15.22 +02:16:00.3
07:21:59.34 -02:01:00.5
06:40:48.78 -00:33:38.5
07:22:32.66 -01:44:04.6
07:09:40.94 -04:22:45.1
06:54:23.70 -04:11:37.9
06:45:28.99 +02:24:20.5
07:08:24.79 +02:46:17.7
07:12:48.84 +01:20:08.9
07:08:57.65 -03:05:11.0
06:51:10.45 +01:06:00.5
07:22:33.94 -00:33:48.1
06:54:45.16 +02:52:16.0
07:07:09.33 -01:15:16.3
07:19:26.37 -01:55:44.5
06:46:13.86 +00:50:45.3
07:04:02.03 +02:51:32.4
07:06:31.68 +02:11:36.3
07:13:29.26 -04:08:39.0
07:11:19.66 -02:24:42.3
07:20:20.02 -01:34:22.0
07:03:38.84 -02:31:45.3
07:10:38.42 -00:26:09.2
07:15:07.42 -00:40:05.2
07:09:45.49 -03:50:37.7
07:07:26.07 -02:04:10.2
07:07:25.92 -01:50:45.1
07:14:00.43 -01:15:31.0
07:04:10.66 -03:14:37.6
07:13:41.67 -03:55:39.1
06:44:27.29 +02:30:55.7
07:00:37.09 +02:24:01.4
07:13:34.27 -04:04:38.4
07:14:59.16 -01:45:25.0
07:18:23.24 +01:03:42.2
07:11:08.09 +00:18:35.8
07:12:47.77 -02:27:16.8
07:17:28.74 -01:41:40.3
07:18:29.75 -00:11:36.0
07:16:55.49 -04:32:30.0
06:56:45.63 +00:46:09.1
06:56:45.10 +00:46:34.7
07:17:15.35 -02:36:55.8
07:13:39.24 +00:17:18.6
07:05:46.99 +00:13:15.3
07:13:03.13 -04:47:14.1
07:07:11.25 -02:58:19.6
07:10:57.64 +01:38:35.0
07:21:06.40 -03:14:57.8
07:15:46.86 -01:58:00.5
07:09:56.39 -04:34:53.5
06:56:02.79 +02:23:22.8
07:14:45.36 -06:00:15.5
07:12:56.17 +02:36:39.4
06:43:50.32 +01:35:50.8
07:00:51.99 +00:12:01.1
07:20:03.58 -01:48:50.5
07:08:11.40 -02:49:43.0
07:15:25.90 -01:11:23.0
07:10:02.55 -02:31:59.1
07:18:12.82 -01:43:03.6
07:01:10.19 +00:00:19.9
06:56:48.94 +00:46:32.8
07:11:37.83 +01:05:41.3
07:04:16.64 -03:01:37.2
07:11:45.29 -05:40:08.5
06:58:35.34 -04:20:25.8
07:05:20.36 +02:45:54.9
07:14:45.29 -01:22:49.3
06:58:50.12 -04:41:10.2
07:04:34.56 -05:56:28.1
06:49:52.97 +02:30:14.8
07:18:29.79 +00:52:08.9
07:19:08.27 -02:01:49.6
07:15:10.04 +00:21:59.8
06:37:16.15 +03:08:57.2
07:15:39.53 -00:49:28.3
07:10:42.55 -01:49:35.9
06:22:43.46 -02:10:03.9
07:17:41.20 +00:07:00.0
07:10:41.81 -02:46:24.7
07:08:10.19 -03:43:12.7
07:14:06.75 +01:28:20.5
07:04:33.73 -04:28:38.5
06:45:39.05 +02:45:24.8
06:36:32.32 -03:35:55.2
07:16:50.04 -03:31:10.0
07:19:06.80 -02:29:52.0
07:21:16.78 -03:12:16.2
06:49:16.17 -06:30:09.0
07:19:50.40 -02:35:19.8
07:05:20.53 +02:02:06.0
07:07:01.92 +00:40:29.5
06:45:09.47 +02:51:11.5
06:54:39.42 +02:38:00.9
07:09:28.97 -06:44:34.8
07:05:49.20 +02:34:31.7
07:10:49.21 -05:23:04.9
07:16:08.09 -03:04:46.8
06:35:10.41 -00:43:19.3
06:49:07.32 -01:40:17.6
07:11:20.02 +01:36:58.4
07:09:24.18 -01:33:15.7
06:58:57.63 +02:32:41.3
07:02:37.62 -01:54:05.5
07:15:16.33 -04:43:31.4
07:16:20.97 -00:19:45.3
06:45:33.70 -00:26:15.8
06:58:35.93 -01:00:30.4
07:12:48.06 +02:19:47.3
07:05:38.60 +01:26:03.2
07:15:49.13 -01:44:51.8
06:24:33.45 -01:26:13.6
07:17:42.14 -00:21:03.7
06:42:30.91 -06:04:21.1
06:46:10.28 -03:13:59.7
07:08:44.77 -01:27:54.2
06:57:35.55 +01:13:54.5
07:10:59.09 -03:24:27.9
07:06:54.08 +02:10:49.3
06:48:33.24 +01:48:58.0
07:01:18.50 -03:25:51.2
06:24:34.49 -01:26:23.8
07:13:40.78 -01:01:26.1
07:04:13.55 +01:59:53.3
07:08:58.12 -02:02:47.5
06:56:39.71 +00:24:11.4
07:15:35.43 +02:02:01.7
07:07:02.56 -00:42:25.6
07:04:32.63 -02:17:38.7
07:17:17.77 -00:03:13.1
07:03:45.85 -02:09:34.0
07:10:10.01 -00:03:44.9
07:03:46.90 -01:04:51.3
06:50:41.49 -00:31:45.0
07:02:23.39 -05:08:56.1
07:08:52.69 -03:55:19.2
07:17:36.38 +00:20:10.6
06:58:22.52 -02:33:47.8
06:32:37.47 -00:21:32.4
07:07:03.67 -02:21:52.0
07:01:49.42 -05:35:31.2
07:11:30.81 -04:56:27.0
06:34:16.11 -05:20:19.0
06:53:13.84 -04:35:47.4
07:17:12.67 +02:26:39.2
07:01:28.02 -05:15:03.7
07:20:44.53 -05:00:15.3
07:21:46.89 -04:08:39.8
06:38:49.79 +02:05:40.6
07:05:52.53 -00:00:59.4
06:38:39.42 +01:56:42.6
06:58:33.92 -01:38:09.5
07:10:03.22 +01:44:56.9
07:06:37.26 +00:11:58.2
06:48:56.93 -03:30:57.1
06:55:44.95 +01:32:28.0
06:46:16.57 +02:25:30.3
07:14:25.25 -06:11:44.0
07:08:01.10 -01:31:58.2
06:58:04.61 +00:51:04.1
07:21:22.39 -05:02:55.9
07:15:31.16 +00:28:43.2
07:07:06.62 +01:52:36.0
07:07:59.65 -00:24:51.6
07:09:36.21 +01:42:30.9
06:53:20.62 +02:43:17.5
07:18:54.14 +01:36:32.4
07:08:49.10 -00:04:32.4
07:18:00.41 -03:35:48.4
07:11:50.14 +01:30:57.6
07:11:49.96 +01:54:46.1
07:00:33.69 -00:05:51.2
07:13:50.70 +01:53:52.8
07:11:23.67 -07:04:29.5
07:16:03.21 +01:36:13.2
07:10:13.28 -01:12:05.9
07:11:38.89 -03:15:42.0
07:13:41.27 -03:39:08.7
07:15:45.85 -02:39:23.4
07:03:00.75 +02:24:11.0
06:58:47.95 -03:05:31.3
07:00:20.05 -02:59:45.0
07:21:26.49 -04:48:08.0
06:47:44.80 +00:19:24.4
07:17:25.27 +02:31:58.2
07:14:29.95 +01:49:08.2
07:13:14.78 -03:26:46.1
07:20:05.61 -00:29:44.4
06:52:19.01 +00:50:19.6
07:21:28.67 -04:04:57.4
07:08:41.07 -03:29:16.1
07:20:29.07 +02:01:14.6
06:55:50.64 -02:12:28.4
07:06:50.68 -03:05:03.4
07:16:41.81 +02:29:08.8
06:57:36.17 +01:03:44.4
07:21:23.98 -00:37:27.2
06:52:34.69 +00:32:34.8
07:14:59.81 +01:48:09.3
07:16:03.06 -00:40:39.8
07:17:35.03 +01:29:52.9
06:52:02.71 +01:24:02.0
07:14:33.99 -05:29:12.2
07:12:55.88 -01:41:31.2
07:16:46.06 -01:27:55.3
07:20:20.06 -00:44:21.3
07:09:36.61 -03:32:25.0
06:51:24.46 +01:46:42.6
07:05:39.86 +02:28:20.2
07:20:37.02 -05:27:07.1
07:14:12.32 -04:54:52.4
07:10:20.63 -00:55:59.4
07:14:23.75 -00:00:49.6
07:01:34.41 +01:46:03.5
06:55:56.27 +02:39:57.3
07:20:05.65 +01:09:50.0
06:30:11.26 +01:52:30.9
07:05:25.56 -02:12:22.9
07:09:37.42 -04:39:36.0
07:12:32.05 +00:04:09.4
07:03:51.50 +02:00:05.0
06:59:46.42 -00:07:54.4
07:10:55.03 -01:45:30.6
07:06:43.05 +01:06:56.7
07:12:07.31 -02:41:42.0
07:08:40.99 -00:53:47.0
07:06:31.61 +02:05:37.7
07:18:14.36 +00:02:43.8
07:05:56.42 -03:14:54.0
07:00:01.63 -04:09:57.6
07:19:23.66 +00:34:09.9
07:04:19.74 +01:39:45.5
06:54:25.05 -00:23:50.1
07:20:55.56 +00:36:26.3
07:12:26.80 +02:04:47.0
07:12:20.26 +01:25:29.4
07:21:03.32 +00:12:22.6
07:05:41.30 +02:40:15.0
07:08:39.92 -02:15:36.2
07:11:29.22 -03:50:43.6
07:13:14.15 -01:39:24.3
07:17:41.55 -02:02:57.4
07:14:46.42 -01:18:37.0
07:13:29.25 -00:50:57.8
07:09:08.35 +00:42:47.5
07:09:13.17 +00:26:49.8
06:42:39.82 +02:05:23.9
07:00:30.73 -02:55:25.7
06:59:37.53 -02:43:47.3
07:11:10.01 +02:18:12.0
07:18:00.81 +00:09:40.9
07:16:14.82 -00:14:34.3
07:13:34.72 -00:26:21.7
06:45:21.84 +02:57:34.8
07:07:59.09 +02:08:45.2
07:12:22.74 -04:42:42.9
07:12:48.01 -00:27:16.3
07:09:12.86 -00:34:11.6
07:17:16.56 -00:42:24.4
07:12:17.34 -01:40:18.5
07:10:33.95 -00:34:04.4
07:14:05.46 +00:33:06.9
07:22:28.38 +00:11:02.8
07:15:08.46 +00:57:32.7
07:13:04.11 -01:16:35.5
07:12:53.04 -00:10:58.7
07:09:52.27 +00:44:50.4
07:10:10.10 +02:03:17.9
07:16:17.04 +01:00:36.5
06:59:22.85 +02:14:38.5
06:47:02.60 +03:07:54.3
07:11:43.64 +02:18:05.1
06:55:40.98 +02:55:19.8
07:11:39.57 -00:20:22.1
07:02:45.30 -04:03:44.7
07:17:46.83 -02:42:16.0
07:02:06.97 -01:14:09.2
07:03:30.37 -03:45:39.9
06:41:48.23 -06:55:07.2
07:17:31.21 +01:05:39.1
06:41:59.22 -01:11:10.0
06:32:07.39 +01:43:00.1
06:27:01.32 -04:35:40.9
06:32:36.12 +00:38:18.8
07:09:11.19 -05:50:47.6
07:08:45.27 +00:41:48.2
06:45:42.35 -04:56:34.2
06:51:26.28 -05:15:26.0
06:52:06.22 -04:01:52.3
07:05:28.64 -02:00:08.1
06:37:53.09 -05:55:16.3
06:44:47.48 -05:17:45.6
###################################################################################
07:09:13.71 -02:21:31.0 -- not an asteroid (will add it to exclusion list)
06:40:30.44 -01:04:41.8 -- not an asteroid (will add it to exclusion list)
06:26:05.11 -03:31:26.5 -- not an asteroid (will add it to exclusion list)
07:05:27.95 +00:36:30.6 -- not an asteroid (will add it to exclusion list)
07:08:51.33 -02:26:19.9 -- not an asteroid (will add it to exclusion list)
06:57:55.39 -00:13:52.7 -- not an asteroid (will add it to exclusion list)
07:11:32.32 +01:26:33.4 -- not an asteroid (will add it to exclusion list)
07:17:45.13 -00:17:16.0 -- not an asteroid (will add it to exclusion list)
07:14:06.90 -04:20:52.6 -- not an asteroid (will add it to exclusion list)
07:13:12.01 +00:38:43.6 -- not an asteroid (will add it to exclusion list)
07:09:04.05 -01:41:57.0 -- not an asteroid (will add it to exclusion list)
07:07:34.54 -03:27:34.7 -- not an asteroid (will add it to exclusion list)
07:01:58.09 -02:16:28.4 -- not an asteroid (will add it to exclusion list)
06:54:14.52 +03:03:39.4 -- not an asteroid (will add it to exclusion list)
07:13:26.54 +00:56:15.8 -- not an asteroid (will add it to exclusion list)
07:14:18.34 -04:09:01.6 -- not an asteroid (will add it to exclusion list)
07:06:56.23 +00:23:23.9 -- not an asteroid (will add it to exclusion list)
06:59:25.19 -01:21:53.4 -- not an asteroid (will add it to exclusion list)
07:08:52.74 -04:21:47.6 -- not an asteroid (will add it to exclusion list)
06:46:26.52 +00:59:02.8 -- not an asteroid (will add it to exclusion list)
07:11:47.40 +01:41:59.3 -- not an asteroid (will add it to exclusion list)
07:05:45.60 -02:32:43.4 -- not an asteroid (will add it to exclusion list)
06:27:32.84 -01:10:22.5 -- not an asteroid (will add it to exclusion list)
07:17:25.66 -04:17:48.9 -- not an asteroid (will add it to exclusion list)
06:55:54.31 +02:54:13.9 -- not an asteroid (will add it to exclusion list)
07:17:32.78 +01:33:25.8 -- not an asteroid (will add it to exclusion list)
07:19:27.98 -02:42:29.5 -- not an asteroid (will add it to exclusion list)
06:49:31.00 +01:58:04.3 -- not an asteroid (will add it to exclusion list)
07:15:27.30 -02:29:46.1 -- not an asteroid (will add it to exclusion list)
06:56:57.91 +00:29:34.9 -- not an asteroid (will add it to exclusion list)
06:55:37.51 +02:46:14.4 -- not an asteroid (will add it to exclusion list)
07:11:19.76 -03:51:44.5 -- not an asteroid (will add it to exclusion list)
07:04:32.14 +00:11:23.7 -- not an asteroid (will add it to exclusion list)
07:09:20.41 +00:20:20.3 -- not an asteroid (will add it to exclusion list)
06:57:22.88 +02:20:21.3 -- not an asteroid (will add it to exclusion list)
06:50:58.57 +01:35:34.5 -- not an asteroid (will add it to exclusion list)
07:16:40.42 -01:23:38.8 -- not an asteroid (will add it to exclusion list)
07:16:08.79 +00:47:13.0 -- not an asteroid (will add it to exclusion list)
07:06:18.03 +01:07:23.6 -- not an asteroid (will add it to exclusion list)
06:43:03.07 -03:21:50.2 -- not an asteroid (will add it to exclusion list)
06:28:19.58 -04:08:29.6 -- not an asteroid (will add it to exclusion list)
07:21:21.93 -00:51:52.0 -- not an asteroid (will add it to exclusion list)
07:22:07.41 -02:10:22.0 -- not an asteroid (will add it to exclusion list)
07:15:05.82 +02:37:23.0 -- not an asteroid (will add it to exclusion list)
07:08:31.17 -00:56:08.8 -- not an asteroid (will add it to exclusion list)
07:02:33.02 +02:20:26.1 -- not an asteroid (will add it to exclusion list)
07:10:48.74 -00:38:30.1 -- not an asteroid (will add it to exclusion list)
07:21:31.52 -01:38:19.3 -- not an asteroid (will add it to exclusion list)
07:20:31.64 -06:57:28.9 -- not an asteroid (will add it to exclusion list)
06:43:46.45 -05:42:08.3 -- not an asteroid (will add it to exclusion list)
07:19:44.76 -03:04:57.8 -- not an asteroid (will add it to exclusion list)
07:19:24.39 -00:41:30.7 -- not an asteroid (will add it to exclusion list)
07:09:37.99 +02:07:35.5 -- not an asteroid (will add it to exclusion list)
07:03:23.58 -00:39:16.9 -- not an asteroid (will add it to exclusion list)
07:16:58.56 +00:50:26.6 -- not an asteroid (will add it to exclusion list)
06:30:15.22 +02:16:00.3 -- not an asteroid (will add it to exclusion list)
07:21:59.34 -02:01:00.5 -- not an asteroid (will add it to exclusion list)
06:40:48.78 -00:33:38.5 -- not an asteroid (will add it to exclusion list)
07:22:32.66 -01:44:04.6 -- not an asteroid (will add it to exclusion list)
07:09:40.94 -04:22:45.1 -- not an asteroid (will add it to exclusion list)
06:54:23.70 -04:11:37.9 -- not an asteroid (will add it to exclusion list)
06:45:28.99 +02:24:20.5 -- not an asteroid (will add it to exclusion list)
07:08:24.79 +02:46:17.7 -- not an asteroid (will add it to exclusion list)
07:12:48.84 +01:20:08.9 -- not an asteroid (will add it to exclusion list)
07:08:57.65 -03:05:11.0 -- not an asteroid (will add it to exclusion list)
06:51:10.45 +01:06:00.5 -- not an asteroid (will add it to exclusion list)
07:22:33.94 -00:33:48.1 -- not an asteroid (will add it to exclusion list)
06:54:45.16 +02:52:16.0 -- not an asteroid (will add it to exclusion list)
07:07:09.33 -01:15:16.3 -- not an asteroid (will add it to exclusion list)
07:19:26.37 -01:55:44.5 -- not an asteroid (will add it to exclusion list)
06:46:13.86 +00:50:45.3 -- not an asteroid (will add it to exclusion list)
07:04:02.03 +02:51:32.4 -- not an asteroid (will add it to exclusion list)
07:06:31.68 +02:11:36.3 -- not an asteroid (will add it to exclusion list)
07:13:29.26 -04:08:39.0 -- not an asteroid (will add it to exclusion list)
07:11:19.66 -02:24:42.3 -- not an asteroid (will add it to exclusion list)
07:20:20.02 -01:34:22.0 -- not an asteroid (will add it to exclusion list)
07:03:38.84 -02:31:45.3 -- not an asteroid (will add it to exclusion list)
07:10:38.42 -00:26:09.2 -- not an asteroid (will add it to exclusion list)
07:15:07.42 -00:40:05.2 -- not an asteroid (will add it to exclusion list)
07:09:45.49 -03:50:37.7 -- not an asteroid (will add it to exclusion list)
07:07:26.07 -02:04:10.2 -- not an asteroid (will add it to exclusion list)
07:07:25.92 -01:50:45.1 -- not an asteroid (will add it to exclusion list)
07:14:00.43 -01:15:31.0 -- not an asteroid (will add it to exclusion list)
07:04:10.66 -03:14:37.6 -- not an asteroid (will add it to exclusion list)
07:13:41.67 -03:55:39.1 -- not an asteroid (will add it to exclusion list)
06:44:27.29 +02:30:55.7 -- not an asteroid (will add it to exclusion list)
07:00:37.09 +02:24:01.4 -- not an asteroid (will add it to exclusion list)
07:13:34.27 -04:04:38.4 -- not an asteroid (will add it to exclusion list)
07:14:59.16 -01:45:25.0 -- not an asteroid (will add it to exclusion list)
07:18:23.24 +01:03:42.2 -- not an asteroid (will add it to exclusion list)
07:11:08.09 +00:18:35.8 -- not an asteroid (will add it to exclusion list)
07:12:47.77 -02:27:16.8 -- not an asteroid (will add it to exclusion list)
07:17:28.74 -01:41:40.3 -- not an asteroid (will add it to exclusion list)
07:18:29.75 -00:11:36.0 -- not an asteroid (will add it to exclusion list)
07:16:55.49 -04:32:30.0 -- not an asteroid (will add it to exclusion list)
06:56:45.63 +00:46:09.1 -- not an asteroid (will add it to exclusion list)
06:56:45.10 +00:46:34.7 -- not an asteroid (will add it to exclusion list)
07:17:15.35 -02:36:55.8 -- not an asteroid (will add it to exclusion list)
07:13:39.24 +00:17:18.6 -- not an asteroid (will add it to exclusion list)
07:05:46.99 +00:13:15.3 -- not an asteroid (will add it to exclusion list)
07:13:03.13 -04:47:14.1 -- not an asteroid (will add it to exclusion list)
07:07:11.25 -02:58:19.6 -- not an asteroid (will add it to exclusion list)
07:10:57.64 +01:38:35.0 -- not an asteroid (will add it to exclusion list)
07:21:06.40 -03:14:57.8 -- not an asteroid (will add it to exclusion list)
07:15:46.86 -01:58:00.5 -- not an asteroid (will add it to exclusion list)
07:09:56.39 -04:34:53.5 -- not an asteroid (will add it to exclusion list)
06:56:02.79 +02:23:22.8 -- not an asteroid (will add it to exclusion list)
07:14:45.36 -06:00:15.5 -- not an asteroid (will add it to exclusion list)
07:12:56.17 +02:36:39.4 -- not an asteroid (will add it to exclusion list)
06:43:50.32 +01:35:50.8 -- not an asteroid (will add it to exclusion list)
07:00:51.99 +00:12:01.1 -- not an asteroid (will add it to exclusion list)
07:20:03.58 -01:48:50.5 -- not an asteroid (will add it to exclusion list)
07:08:11.40 -02:49:43.0 -- not an asteroid (will add it to exclusion list)
07:15:25.90 -01:11:23.0 -- not an asteroid (will add it to exclusion list)
07:10:02.55 -02:31:59.1 -- not an asteroid (will add it to exclusion list)
07:18:12.82 -01:43:03.6 -- not an asteroid (will add it to exclusion list)
07:01:10.19 +00:00:19.9 -- not an asteroid (will add it to exclusion list)
06:56:48.94 +00:46:32.8 -- not an asteroid (will add it to exclusion list)
07:11:37.83 +01:05:41.3 -- not an asteroid (will add it to exclusion list)
07:04:16.64 -03:01:37.2 -- not an asteroid (will add it to exclusion list)
07:11:45.29 -05:40:08.5 -- not an asteroid (will add it to exclusion list)
06:58:35.34 -04:20:25.8 -- not an asteroid (will add it to exclusion list)
07:05:20.36 +02:45:54.9 -- not an asteroid (will add it to exclusion list)
07:14:45.29 -01:22:49.3 -- not an asteroid (will add it to exclusion list)
06:58:50.12 -04:41:10.2 -- not an asteroid (will add it to exclusion list)
07:04:34.56 -05:56:28.1 -- not an asteroid (will add it to exclusion list)
06:49:52.97 +02:30:14.8 -- not an asteroid (will add it to exclusion list)
07:18:29.79 +00:52:08.9 -- not an asteroid (will add it to exclusion list)
07:19:08.27 -02:01:49.6 -- not an asteroid (will add it to exclusion list)
07:15:10.04 +00:21:59.8 -- not an asteroid (will add it to exclusion list)
06:37:16.15 +03:08:57.2 -- not an asteroid (will add it to exclusion list)
07:15:39.53 -00:49:28.3 -- not an asteroid (will add it to exclusion list)
07:10:42.55 -01:49:35.9 -- not an asteroid (will add it to exclusion list)
06:22:43.46 -02:10:03.9 -- not an asteroid (will add it to exclusion list)
07:17:41.20 +00:07:00.0 -- not an asteroid (will add it to exclusion list)
07:10:41.81 -02:46:24.7 -- not an asteroid (will add it to exclusion list)
07:08:10.19 -03:43:12.7 -- not an asteroid (will add it to exclusion list)
07:14:06.75 +01:28:20.5 -- not an asteroid (will add it to exclusion list)
07:04:33.73 -04:28:38.5 -- not an asteroid (will add it to exclusion list)
06:45:39.05 +02:45:24.8 -- not an asteroid (will add it to exclusion list)
06:36:32.32 -03:35:55.2 -- not an asteroid (will add it to exclusion list)
07:16:50.04 -03:31:10.0 -- not an asteroid (will add it to exclusion list)
07:19:06.80 -02:29:52.0 -- not an asteroid (will add it to exclusion list)
07:21:16.78 -03:12:16.2 -- not an asteroid (will add it to exclusion list)
06:49:16.17 -06:30:09.0 -- not an asteroid (will add it to exclusion list)
07:19:50.40 -02:35:19.8 -- not an asteroid (will add it to exclusion list)
07:05:20.53 +02:02:06.0 -- not an asteroid (will add it to exclusion list)
07:07:01.92 +00:40:29.5 -- not an asteroid (will add it to exclusion list)
06:45:09.47 +02:51:11.5 -- not an asteroid (will add it to exclusion list)
06:54:39.42 +02:38:00.9 -- not an asteroid (will add it to exclusion list)
07:09:28.97 -06:44:34.8 -- not an asteroid (will add it to exclusion list)
07:05:49.20 +02:34:31.7 -- not an asteroid (will add it to exclusion list)
07:10:49.21 -05:23:04.9 -- not an asteroid (will add it to exclusion list)
07:16:08.09 -03:04:46.8 -- not an asteroid (will add it to exclusion list)
06:35:10.41 -00:43:19.3 -- not an asteroid (will add it to exclusion list)
06:49:07.32 -01:40:17.6 -- not an asteroid (will add it to exclusion list)
07:11:20.02 +01:36:58.4 -- not an asteroid (will add it to exclusion list)
07:09:24.18 -01:33:15.7 -- not an asteroid (will add it to exclusion list)
06:58:57.63 +02:32:41.3 -- not an asteroid (will add it to exclusion list)
07:02:37.62 -01:54:05.5 -- not an asteroid (will add it to exclusion list)
07:15:16.33 -04:43:31.4 -- not an asteroid (will add it to exclusion list)
07:16:20.97 -00:19:45.3 -- not an asteroid (will add it to exclusion list)
06:45:33.70 -00:26:15.8 -- not an asteroid (will add it to exclusion list)
06:58:35.93 -01:00:30.4 -- not an asteroid (will add it to exclusion list)
07:12:48.06 +02:19:47.3 -- not an asteroid (will add it to exclusion list)
07:05:38.60 +01:26:03.2 -- not an asteroid (will add it to exclusion list)
07:15:49.13 -01:44:51.8 -- not an asteroid (will add it to exclusion list)
06:24:33.45 -01:26:13.6 -- not an asteroid (will add it to exclusion list)
07:17:42.14 -00:21:03.7 -- not an asteroid (will add it to exclusion list)
06:42:30.91 -06:04:21.1 -- not an asteroid (will add it to exclusion list)
06:46:10.28 -03:13:59.7 -- not an asteroid (will add it to exclusion list)
07:08:44.77 -01:27:54.2 -- not an asteroid (will add it to exclusion list)
06:57:35.55 +01:13:54.5 -- not an asteroid (will add it to exclusion list)
07:10:59.09 -03:24:27.9 -- not an asteroid (will add it to exclusion list)
07:06:54.08 +02:10:49.3 -- not an asteroid (will add it to exclusion list)
06:48:33.24 +01:48:58.0 -- not an asteroid (will add it to exclusion list)
07:01:18.50 -03:25:51.2 -- not an asteroid (will add it to exclusion list)
06:24:34.49 -01:26:23.8 -- not an asteroid (will add it to exclusion list)
07:13:40.78 -01:01:26.1 -- not an asteroid (will add it to exclusion list)
07:04:13.55 +01:59:53.3 -- not an asteroid (will add it to exclusion list)
07:08:58.12 -02:02:47.5 -- not an asteroid (will add it to exclusion list)
06:56:39.71 +00:24:11.4 -- not an asteroid (will add it to exclusion list)
07:15:35.43 +02:02:01.7 -- not an asteroid (will add it to exclusion list)
07:07:02.56 -00:42:25.6 -- not an asteroid (will add it to exclusion list)
07:04:32.63 -02:17:38.7 -- not an asteroid (will add it to exclusion list)
07:17:17.77 -00:03:13.1 -- not an asteroid (will add it to exclusion list)
07:03:45.85 -02:09:34.0 -- not an asteroid (will add it to exclusion list)
07:10:10.01 -00:03:44.9 -- not an asteroid (will add it to exclusion list)
07:03:46.90 -01:04:51.3 -- not an asteroid (will add it to exclusion list)
06:50:41.49 -00:31:45.0 -- not an asteroid (will add it to exclusion list)
07:02:23.39 -05:08:56.1 -- not an asteroid (will add it to exclusion list)
07:08:52.69 -03:55:19.2 -- not an asteroid (will add it to exclusion list)
07:17:36.38 +00:20:10.6 -- not an asteroid (will add it to exclusion list)
06:58:22.52 -02:33:47.8 -- not an asteroid (will add it to exclusion list)
06:32:37.47 -00:21:32.4 -- not an asteroid (will add it to exclusion list)
07:07:03.67 -02:21:52.0 -- not an asteroid (will add it to exclusion list)
07:01:49.42 -05:35:31.2 -- not an asteroid (will add it to exclusion list)
07:11:30.81 -04:56:27.0 -- not an asteroid (will add it to exclusion list)
06:34:16.11 -05:20:19.0 -- not an asteroid (will add it to exclusion list)
06:53:13.84 -04:35:47.4 -- not an asteroid (will add it to exclusion list)
07:17:12.67 +02:26:39.2 -- not an asteroid (will add it to exclusion list)
07:01:28.02 -05:15:03.7 -- not an asteroid (will add it to exclusion list)
07:20:44.53 -05:00:15.3 -- not an asteroid (will add it to exclusion list)
07:21:46.89 -04:08:39.8 -- not an asteroid (will add it to exclusion list)
06:38:49.79 +02:05:40.6 -- not an asteroid (will add it to exclusion list)
07:05:52.53 -00:00:59.4 -- not an asteroid (will add it to exclusion list)
06:38:39.42 +01:56:42.6 -- not an asteroid (will add it to exclusion list)
06:58:33.92 -01:38:09.5 -- not an asteroid (will add it to exclusion list)
07:10:03.22 +01:44:56.9 -- not an asteroid (will add it to exclusion list)
07:06:37.26 +00:11:58.2 -- not an asteroid (will add it to exclusion list)
06:48:56.93 -03:30:57.1 -- not an asteroid (will add it to exclusion list)
06:55:44.95 +01:32:28.0 -- not an asteroid (will add it to exclusion list)
06:46:16.57 +02:25:30.3 -- not an asteroid (will add it to exclusion list)
07:14:25.25 -06:11:44.0 -- not an asteroid (will add it to exclusion list)
07:08:01.10 -01:31:58.2 -- not an asteroid (will add it to exclusion list)
06:58:04.61 +00:51:04.1 -- not an asteroid (will add it to exclusion list)
07:21:22.39 -05:02:55.9 -- not an asteroid (will add it to exclusion list)
07:15:31.16 +00:28:43.2 -- not an asteroid (will add it to exclusion list)
07:07:06.62 +01:52:36.0 -- not an asteroid (will add it to exclusion list)
07:07:59.65 -00:24:51.6 -- not an asteroid (will add it to exclusion list)
07:09:36.21 +01:42:30.9 -- not an asteroid (will add it to exclusion list)
06:53:20.62 +02:43:17.5 -- not an asteroid (will add it to exclusion list)
07:18:54.14 +01:36:32.4 -- not an asteroid (will add it to exclusion list)
07:08:49.10 -00:04:32.4 -- not an asteroid (will add it to exclusion list)
07:18:00.41 -03:35:48.4 -- not an asteroid (will add it to exclusion list)
07:11:50.14 +01:30:57.6 -- not an asteroid (will add it to exclusion list)
07:11:49.96 +01:54:46.1 -- not an asteroid (will add it to exclusion list)
07:00:33.69 -00:05:51.2 -- not an asteroid (will add it to exclusion list)
07:13:50.70 +01:53:52.8 -- not an asteroid (will add it to exclusion list)
07:11:23.67 -07:04:29.5 -- not an asteroid (will add it to exclusion list)
07:16:03.21 +01:36:13.2 -- not an asteroid (will add it to exclusion list)
07:10:13.28 -01:12:05.9 -- not an asteroid (will add it to exclusion list)
07:11:38.89 -03:15:42.0 -- not an asteroid (will add it to exclusion list)
07:13:41.27 -03:39:08.7 -- not an asteroid (will add it to exclusion list)
07:15:45.85 -02:39:23.4 -- not an asteroid (will add it to exclusion list)
07:03:00.75 +02:24:11.0 -- not an asteroid (will add it to exclusion list)
06:58:47.95 -03:05:31.3 -- not an asteroid (will add it to exclusion list)
07:00:20.05 -02:59:45.0 -- not an asteroid (will add it to exclusion list)
07:21:26.49 -04:48:08.0 -- not an asteroid (will add it to exclusion list)
06:47:44.80 +00:19:24.4 -- not an asteroid (will add it to exclusion list)
07:17:25.27 +02:31:58.2 -- not an asteroid (will add it to exclusion list)
07:14:29.95 +01:49:08.2 -- not an asteroid (will add it to exclusion list)
07:13:14.78 -03:26:46.1 -- not an asteroid (will add it to exclusion list)
07:20:05.61 -00:29:44.4 -- not an asteroid (will add it to exclusion list)
06:52:19.01 +00:50:19.6 -- not an asteroid (will add it to exclusion list)
07:21:28.67 -04:04:57.4 -- not an asteroid (will add it to exclusion list)
07:08:41.07 -03:29:16.1 -- not an asteroid (will add it to exclusion list)
07:20:29.07 +02:01:14.6 -- not an asteroid (will add it to exclusion list)
06:55:50.64 -02:12:28.4 -- not an asteroid (will add it to exclusion list)
07:06:50.68 -03:05:03.4 -- not an asteroid (will add it to exclusion list)
07:16:41.81 +02:29:08.8 -- not an asteroid (will add it to exclusion list)
06:57:36.17 +01:03:44.4 -- not an asteroid (will add it to exclusion list)
07:21:23.98 -00:37:27.2 -- not an asteroid (will add it to exclusion list)
06:52:34.69 +00:32:34.8 -- not an asteroid (will add it to exclusion list)
07:14:59.81 +01:48:09.3 -- not an asteroid (will add it to exclusion list)
07:16:03.06 -00:40:39.8 -- not an asteroid (will add it to exclusion list)
07:17:35.03 +01:29:52.9 -- not an asteroid (will add it to exclusion list)
06:52:02.71 +01:24:02.0 -- not an asteroid (will add it to exclusion list)
07:14:33.99 -05:29:12.2 -- not an asteroid (will add it to exclusion list)
07:12:55.88 -01:41:31.2 -- not an asteroid (will add it to exclusion list)
07:16:46.06 -01:27:55.3 -- not an asteroid (will add it to exclusion list)
07:20:20.06 -00:44:21.3 -- not an asteroid (will add it to exclusion list)
07:09:36.61 -03:32:25.0 -- not an asteroid (will add it to exclusion list)
06:51:24.46 +01:46:42.6 -- not an asteroid (will add it to exclusion list)
07:05:39.86 +02:28:20.2 -- not an asteroid (will add it to exclusion list)
07:20:37.02 -05:27:07.1 -- not an asteroid (will add it to exclusion list)
07:14:12.32 -04:54:52.4 -- not an asteroid (will add it to exclusion list)
07:10:20.63 -00:55:59.4 -- not an asteroid (will add it to exclusion list)
07:14:23.75 -00:00:49.6 -- not an asteroid (will add it to exclusion list)
07:01:34.41 +01:46:03.5 -- not an asteroid (will add it to exclusion list)
06:55:56.27 +02:39:57.3 -- not an asteroid (will add it to exclusion list)
07:20:05.65 +01:09:50.0 -- not an asteroid (will add it to exclusion list)
06:30:11.26 +01:52:30.9 -- not an asteroid (will add it to exclusion list)
07:05:25.56 -02:12:22.9 -- not an asteroid (will add it to exclusion list)
07:09:37.42 -04:39:36.0 -- not an asteroid (will add it to exclusion list)
07:12:32.05 +00:04:09.4 -- not an asteroid (will add it to exclusion list)
07:03:51.50 +02:00:05.0 -- not an asteroid (will add it to exclusion list)
06:59:46.42 -00:07:54.4 -- not an asteroid (will add it to exclusion list)
07:10:55.03 -01:45:30.6 -- not an asteroid (will add it to exclusion list)
07:06:43.05 +01:06:56.7 -- not an asteroid (will add it to exclusion list)
07:12:07.31 -02:41:42.0 -- not an asteroid (will add it to exclusion list)
07:08:40.99 -00:53:47.0 -- not an asteroid (will add it to exclusion list)
07:06:31.61 +02:05:37.7 -- not an asteroid (will add it to exclusion list)
07:18:14.36 +00:02:43.8 -- not an asteroid (will add it to exclusion list)
07:05:56.42 -03:14:54.0 -- not an asteroid (will add it to exclusion list)
07:00:01.63 -04:09:57.6 -- not an asteroid (will add it to exclusion list)
07:19:23.66 +00:34:09.9 -- not an asteroid (will add it to exclusion list)
07:04:19.74 +01:39:45.5 -- not an asteroid (will add it to exclusion list)
06:54:25.05 -00:23:50.1 -- not an asteroid (will add it to exclusion list)
07:20:55.56 +00:36:26.3 -- not an asteroid (will add it to exclusion list)
07:12:26.80 +02:04:47.0 -- not an asteroid (will add it to exclusion list)
07:12:20.26 +01:25:29.4 -- not an asteroid (will add it to exclusion list)
07:21:03.32 +00:12:22.6 -- not an asteroid (will add it to exclusion list)
07:05:41.30 +02:40:15.0 -- not an asteroid (will add it to exclusion list)
07:08:39.92 -02:15:36.2 -- not an asteroid (will add it to exclusion list)
07:11:29.22 -03:50:43.6 -- not an asteroid (will add it to exclusion list)
07:13:14.15 -01:39:24.3 -- not an asteroid (will add it to exclusion list)
07:17:41.55 -02:02:57.4 -- not an asteroid (will add it to exclusion list)
07:14:46.42 -01:18:37.0 -- not an asteroid (will add it to exclusion list)
07:13:29.25 -00:50:57.8 -- not an asteroid (will add it to exclusion list)
07:09:08.35 +00:42:47.5 -- not an asteroid (will add it to exclusion list)
07:09:13.17 +00:26:49.8 -- not an asteroid (will add it to exclusion list)
06:42:39.82 +02:05:23.9 -- not an asteroid (will add it to exclusion list)
07:00:30.73 -02:55:25.7 -- not an asteroid (will add it to exclusion list)
06:59:37.53 -02:43:47.3 -- not an asteroid (will add it to exclusion list)
07:11:10.01 +02:18:12.0 -- not an asteroid (will add it to exclusion list)
07:18:00.81 +00:09:40.9 -- not an asteroid (will add it to exclusion list)
07:16:14.82 -00:14:34.3 -- not an asteroid (will add it to exclusion list)
07:13:34.72 -00:26:21.7 -- not an asteroid (will add it to exclusion list)
06:45:21.84 +02:57:34.8 -- not an asteroid (will add it to exclusion list)
07:07:59.09 +02:08:45.2 -- not an asteroid (will add it to exclusion list)
07:12:22.74 -04:42:42.9 -- not an asteroid (will add it to exclusion list)
07:12:48.01 -00:27:16.3 -- not an asteroid (will add it to exclusion list)
07:09:12.86 -00:34:11.6 -- not an asteroid (will add it to exclusion list)
07:17:16.56 -00:42:24.4 -- not an asteroid (will add it to exclusion list)
07:12:17.34 -01:40:18.5 -- not an asteroid (will add it to exclusion list)
07:10:33.95 -00:34:04.4 -- not an asteroid (will add it to exclusion list)
07:14:05.46 +00:33:06.9 -- not an asteroid (will add it to exclusion list)
07:22:28.38 +00:11:02.8 -- not an asteroid (will add it to exclusion list)
07:15:08.46 +00:57:32.7 -- not an asteroid (will add it to exclusion list)
07:13:04.11 -01:16:35.5 -- not an asteroid (will add it to exclusion list)
07:12:53.04 -00:10:58.7 -- not an asteroid (will add it to exclusion list)
07:09:52.27 +00:44:50.4 -- not an asteroid (will add it to exclusion list)
07:10:10.10 +02:03:17.9 -- not an asteroid (will add it to exclusion list)
07:16:17.04 +01:00:36.5 -- not an asteroid (will add it to exclusion list)
06:59:22.85 +02:14:38.5 -- not an asteroid (will add it to exclusion list)
06:47:02.60 +03:07:54.3 -- not an asteroid (will add it to exclusion list)
07:11:43.64 +02:18:05.1 -- not an asteroid (will add it to exclusion list)
06:55:40.98 +02:55:19.8 -- not an asteroid (will add it to exclusion list)
07:11:39.57 -00:20:22.1 -- not an asteroid (will add it to exclusion list)
07:02:45.30 -04:03:44.7 -- not an asteroid (will add it to exclusion list)
07:17:46.83 -02:42:16.0 -- not an asteroid (will add it to exclusion list)
07:02:06.97 -01:14:09.2 -- not an asteroid (will add it to exclusion list)
07:03:30.37 -03:45:39.9 -- not an asteroid (will add it to exclusion list)
06:41:48.23 -06:55:07.2 -- not an asteroid (will add it to exclusion list)
07:17:31.21 +01:05:39.1 -- not an asteroid (will add it to exclusion list)
06:41:59.22 -01:11:10.0 -- not an asteroid (will add it to exclusion list)
06:32:07.39 +01:43:00.1 -- not an asteroid (will add it to exclusion list)
06:27:01.32 -04:35:40.9 -- not an asteroid (will add it to exclusion list)
06:32:36.12 +00:38:18.8 -- not an asteroid (will add it to exclusion list)
07:09:11.19 -05:50:47.6 -- not an asteroid (will add it to exclusion list)
07:08:45.27 +00:41:48.2 -- not an asteroid (will add it to exclusion list)
06:45:42.35 -04:56:34.2 -- not an asteroid (will add it to exclusion list)
06:51:26.28 -05:15:26.0 -- not an asteroid (will add it to exclusion list)
06:52:06.22 -04:01:52.3 -- not an asteroid (will add it to exclusion list)
07:05:28.64 -02:00:08.1 -- not an asteroid (will add it to exclusion list)
06:37:53.09 -05:55:16.3 -- not an asteroid (will add it to exclusion list)
06:44:47.48 -05:17:45.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:22:43.46 -02:10:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:33.45 -01:26:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:34.49 -01:26:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:05.11 -03:31:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:01.32 -04:35:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:32.84 -01:10:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:19.58 -04:08:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:11.26 +01:52:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:15.22 +02:16:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:07.39 +01:43:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:36.12 +00:38:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:37.47 -00:21:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:16.11 -05:20:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:10.41 -00:43:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:32.32 -03:35:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:16.15 +03:08:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:53.09 -05:55:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:39.42 +01:56:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:49.79 +02:05:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.44 -01:04:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:48.78 -00:33:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:48.23 -06:55:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:59.22 -01:11:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.91 -06:04:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:39.82 +02:05:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:03.07 -03:21:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.45 -05:42:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:50.32 +01:35:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:27.29 +02:30:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:47.48 -05:17:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:09.47 +02:51:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:21.84 +02:57:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:28.99 +02:24:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.70 -00:26:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.05 +02:45:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:42.35 -04:56:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.28 -03:13:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.86 +00:50:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:16.57 +02:25:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:26.52 +00:59:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:02.60 +03:07:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:44.80 +00:19:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:33.24 +01:48:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:56.93 -03:30:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.32 -01:40:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:16.17 -06:30:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:31.00 +01:58:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.97 +02:30:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.49 -00:31:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:58.57 +01:35:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.45 +01:06:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:24.46 +01:46:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:26.28 -05:15:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:02.71 +01:24:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.22 -04:01:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:19.01 +00:50:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:34.69 +00:32:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:13.84 -04:35:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:20.62 +02:43:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:14.52 +03:03:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:23.70 -04:11:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:25.05 -00:23:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.42 +02:38:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:45.16 +02:52:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:37.51 +02:46:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:40.98 +02:55:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:44.95 +01:32:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.64 -02:12:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:54.31 +02:54:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:56.27 +02:39:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:02.79 +02:23:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:39.71 +00:24:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.10 +00:46:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.63 +00:46:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:48.94 +00:46:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:57.91 +00:29:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:22.88 +02:20:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.55 +01:13:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:36.17 +01:03:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.39 -00:13:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:04.61 +00:51:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.52 -02:33:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:33.92 -01:38:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.34 -04:20:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.93 -01:00:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:47.95 -03:05:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.12 -04:41:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.63 +02:32:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:22.85 +02:14:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:25.19 -01:21:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:37.53 -02:43:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:46.42 -00:07:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.63 -04:09:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:20.05 -02:59:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:30.73 -02:55:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:33.69 -00:05:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:37.09 +02:24:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.99 +00:12:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.19 +00:00:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:18.50 -03:25:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:28.02 -05:15:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:34.41 +01:46:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:49.42 -05:35:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:58.09 -02:16:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:06.97 -01:14:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.39 -05:08:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:33.02 +02:20:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:37.62 -01:54:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:45.30 -04:03:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:00.75 +02:24:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:23.58 -00:39:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:30.37 -03:45:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:38.84 -02:31:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:45.85 -02:09:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:46.90 -01:04:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:51.50 +02:00:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:02.03 +02:51:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.66 -03:14:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:13.55 +01:59:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.64 -03:01:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:19.74 +01:39:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:32.14 +00:11:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:32.63 -02:17:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:33.73 -04:28:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:34.56 -05:56:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.36 +02:45:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.53 +02:02:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:25.56 -02:12:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:27.95 +00:36:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:28.64 -02:00:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.60 +01:26:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:39.86 +02:28:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.30 +02:40:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.60 -02:32:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:46.99 +00:13:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:49.20 +02:34:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:52.53 -00:00:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:56.42 -03:14:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:18.03 +01:07:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.61 +02:05:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.68 +02:11:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:37.26 +00:11:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:43.05 +01:06:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:50.68 -03:05:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.08 +02:10:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:56.23 +00:23:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:01.92 +00:40:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:02.56 -00:42:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:03.67 -02:21:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.62 +01:52:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:09.33 -01:15:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.25 -02:58:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:25.92 -01:50:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.07 -02:04:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:34.54 -03:27:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:59.09 +02:08:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:59.65 -00:24:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:01.10 -01:31:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:10.19 -03:43:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:11.40 -02:49:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:24.79 +02:46:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:31.17 -00:56:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:39.92 -02:15:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:40.99 -00:53:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:41.07 -03:29:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.77 -01:27:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.27 +00:41:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:49.10 -00:04:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:51.33 -02:26:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:52.69 -03:55:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:52.74 -04:21:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:57.65 -03:05:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:58.12 -02:02:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:04.05 -01:41:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.35 +00:42:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:11.19 -05:50:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:12.86 -00:34:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.17 +00:26:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.71 -02:21:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.41 +00:20:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:24.18 -01:33:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:28.97 -06:44:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:36.21 +01:42:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:36.61 -03:32:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:37.42 -04:39:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:37.99 +02:07:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:40.94 -04:22:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:45.49 -03:50:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:52.27 +00:44:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:56.39 -04:34:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:02.55 -02:31:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:03.22 +01:44:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.01 -00:03:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.10 +02:03:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:13.28 -01:12:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:20.63 -00:55:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:33.95 -00:34:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:38.42 -00:26:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:41.81 -02:46:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:42.55 -01:49:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:48.74 -00:38:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:49.21 -05:23:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:55.03 -01:45:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:57.64 +01:38:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:59.09 -03:24:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:08.09 +00:18:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:10.01 +02:18:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.66 -02:24:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.76 -03:51:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:20.02 +01:36:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:23.67 -07:04:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:29.22 -03:50:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:30.81 -04:56:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:32.32 +01:26:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:37.83 +01:05:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:38.89 -03:15:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:39.57 -00:20:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:43.64 +02:18:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:45.29 -05:40:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:47.40 +01:41:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:49.96 +01:54:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:50.14 +01:30:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:07.31 -02:41:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:17.34 -01:40:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:20.26 +01:25:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:22.74 -04:42:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:26.80 +02:04:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:32.05 +00:04:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:47.77 -02:27:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:48.01 -00:27:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:48.06 +02:19:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:48.84 +01:20:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:53.04 -00:10:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:55.88 -01:41:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.17 +02:36:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:03.13 -04:47:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:04.11 -01:16:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:12.01 +00:38:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:14.15 -01:39:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:14.78 -03:26:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:26.54 +00:56:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:29.25 -00:50:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:29.26 -04:08:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:34.27 -04:04:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:34.72 -00:26:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:39.24 +00:17:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:40.78 -01:01:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:41.27 -03:39:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:41.67 -03:55:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:50.70 +01:53:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:00.43 -01:15:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:05.46 +00:33:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:06.75 +01:28:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:06.90 -04:20:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:12.32 -04:54:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:18.34 -04:09:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:23.75 -00:00:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:25.25 -06:11:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:29.95 +01:49:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:33.99 -05:29:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:45.29 -01:22:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:45.36 -06:00:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:46.42 -01:18:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:59.16 -01:45:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:59.81 +01:48:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:05.82 +02:37:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:07.42 -00:40:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:08.46 +00:57:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:10.04 +00:21:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:16.33 -04:43:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:25.90 -01:11:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:27.30 -02:29:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:31.16 +00:28:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:35.43 +02:02:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:39.53 -00:49:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:45.85 -02:39:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:46.86 -01:58:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:49.13 -01:44:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.06 -00:40:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.21 +01:36:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:08.09 -03:04:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:08.79 +00:47:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:14.82 -00:14:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:17.04 +01:00:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:20.97 -00:19:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:40.42 -01:23:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:41.81 +02:29:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:46.06 -01:27:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:50.04 -03:31:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:55.49 -04:32:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:58.56 +00:50:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:12.67 +02:26:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:15.35 -02:36:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:16.56 -00:42:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:17.77 -00:03:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:25.27 +02:31:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:25.66 -04:17:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:28.74 -01:41:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.21 +01:05:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:32.78 +01:33:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:35.03 +01:29:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:36.38 +00:20:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:41.20 +00:07:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:41.55 -02:02:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:42.14 -00:21:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:45.13 -00:17:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:46.83 -02:42:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:00.41 -03:35:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:00.81 +00:09:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:12.82 -01:43:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:14.36 +00:02:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:23.24 +01:03:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:29.75 -00:11:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:29.79 +00:52:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:54.14 +01:36:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:06.80 -02:29:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:08.27 -02:01:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:23.66 +00:34:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:24.39 -00:41:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:26.37 -01:55:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:27.98 -02:42:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:44.76 -03:04:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:50.40 -02:35:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:03.58 -01:48:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:05.61 -00:29:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:05.65 +01:09:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:20.02 -01:34:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:20.06 -00:44:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:29.07 +02:01:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:31.64 -06:57:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:37.02 -05:27:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:44.53 -05:00:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:55.56 +00:36:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:03.32 +00:12:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:06.40 -03:14:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:16.78 -03:12:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:21.93 -00:51:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:22.39 -05:02:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:23.98 -00:37:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:26.49 -04:48:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:28.67 -04:04:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:31.52 -01:38:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:46.89 -04:08:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:59.34 -02:01:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:07.41 -02:10:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:28.38 +00:11:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:32.66 -01:44:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:33.94 -00:33:48.1 -- 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)
06:22:43.46 -02:10:03.9 -- a known variable star
06:24:33.45 -01:26:13.6 -- a known variable star
06:24:34.49 -01:26:23.8 -- a known variable star
06:26:05.11 -03:31:26.5 -- not a known variable star
06:27:01.32 -04:35:40.9 -- a known variable star
06:27:32.84 -01:10:22.5 -- not a known variable star
06:28:19.58 -04:08:29.6 -- not a known variable star
06:30:11.26 +01:52:30.9 -- not a known variable star
06:30:15.22 +02:16:00.3 -- not a known variable star
06:32:07.39 +01:43:00.1 -- a known variable star
06:32:36.12 +00:38:18.8 -- a known variable star
06:32:37.47 -00:21:32.4 -- not a known variable star
06:34:16.11 -05:20:19.0 -- not a known variable star
06:35:10.41 -00:43:19.3 -- not a known variable star
06:36:32.32 -03:35:55.2 -- not a known variable star
06:37:16.15 +03:08:57.2 -- not a known variable star
06:37:53.09 -05:55:16.3 -- a known variable star
06:38:39.42 +01:56:42.6 -- not a known variable star
06:38:49.79 +02:05:40.6 -- a known variable star
06:40:30.44 -01:04:41.8 -- a known variable star
06:40:48.78 -00:33:38.5 -- a known variable star
06:41:48.23 -06:55:07.2 -- not a known variable star
06:41:59.22 -01:11:10.0 -- a known variable star
06:42:30.91 -06:04:21.1 -- a known variable star
06:42:39.82 +02:05:23.9 -- not a known variable star
06:43:03.07 -03:21:50.2 -- not a known variable star
06:43:46.45 -05:42:08.3 -- not a known variable star
06:43:50.32 +01:35:50.8 -- not a known variable star
06:44:27.29 +02:30:55.7 -- not a known variable star
06:44:47.48 -05:17:45.6 -- a known variable star
06:45:09.47 +02:51:11.5 -- a known variable star
06:45:21.84 +02:57:34.8 -- a known variable star
06:45:28.99 +02:24:20.5 -- not a known variable star
06:45:33.70 -00:26:15.8 -- a known variable star
06:45:39.05 +02:45:24.8 -- a known variable star
06:45:42.35 -04:56:34.2 -- a known variable star
06:46:10.28 -03:13:59.7 -- a known variable star
06:46:13.86 +00:50:45.3 -- not a known variable star
06:46:16.57 +02:25:30.3 -- a known variable star
06:46:26.52 +00:59:02.8 -- not a known variable star
06:47:02.60 +03:07:54.3 -- not a known variable star
06:47:44.80 +00:19:24.4 -- not a known variable star
06:48:33.24 +01:48:58.0 -- a known variable star
06:48:56.93 -03:30:57.1 -- not a known variable star
06:49:07.32 -01:40:17.6 -- not a known variable star
06:49:16.17 -06:30:09.0 -- not a known variable star
06:49:31.00 +01:58:04.3 -- not a known variable star
06:49:52.97 +02:30:14.8 -- a known variable star
06:50:41.49 -00:31:45.0 -- not a known variable star
06:50:58.57 +01:35:34.5 -- not a known variable star
06:51:10.45 +01:06:00.5 -- not a known variable star
06:51:24.46 +01:46:42.6 -- not a known variable star
06:51:26.28 -05:15:26.0 -- a known variable star
06:52:02.71 +01:24:02.0 -- not a known variable star
06:52:06.22 -04:01:52.3 -- a known variable star
06:52:19.01 +00:50:19.6 -- not a known variable star
06:52:34.69 +00:32:34.8 -- not a known variable star
06:53:13.84 -04:35:47.4 -- not a known variable star
06:53:20.62 +02:43:17.5 -- not a known variable star
06:54:14.52 +03:03:39.4 -- not a known variable star
06:54:23.70 -04:11:37.9 -- not a known variable star
06:54:25.05 -00:23:50.1 -- not a known variable star
06:54:39.42 +02:38:00.9 -- not a known variable star
06:54:45.16 +02:52:16.0 -- not a known variable star
06:55:37.51 +02:46:14.4 -- a known variable star
06:55:40.98 +02:55:19.8 -- not a known variable star
06:55:44.95 +01:32:28.0 -- a known variable star
06:55:50.64 -02:12:28.4 -- not a known variable star
06:55:54.31 +02:54:13.9 -- not a known variable star
06:55:56.27 +02:39:57.3 -- a known variable star
06:56:02.79 +02:23:22.8 -- not a known variable star
06:56:39.71 +00:24:11.4 -- not a known variable star
06:56:45.10 +00:46:34.7 -- not a known variable star
06:56:45.63 +00:46:09.1 -- not a known variable star
06:56:48.94 +00:46:32.8 -- not a known variable star
06:56:57.91 +00:29:34.9 -- not a known variable star
06:57:22.88 +02:20:21.3 -- not a known variable star
06:57:35.55 +01:13:54.5 -- a known variable star
06:57:36.17 +01:03:44.4 -- not a known variable star
06:57:55.39 -00:13:52.7 -- not a known variable star
06:58:04.61 +00:51:04.1 -- not a known variable star
06:58:22.52 -02:33:47.8 -- a known variable star
06:58:33.92 -01:38:09.5 -- not a known variable star
06:58:35.34 -04:20:25.8 -- not a known variable star
06:58:35.93 -01:00:30.4 -- not a known variable star
06:58:47.95 -03:05:31.3 -- not a known variable star
06:58:50.12 -04:41:10.2 -- not a known variable star
06:58:57.63 +02:32:41.3 -- not a known variable star
06:59:22.85 +02:14:38.5 -- not a known variable star
06:59:25.19 -01:21:53.4 -- not a known variable star
06:59:37.53 -02:43:47.3 -- a known variable star
06:59:46.42 -00:07:54.4 -- not a known variable star
07:00:01.63 -04:09:57.6 -- not a known variable star
07:00:20.05 -02:59:45.0 -- not a known variable star
07:00:30.73 -02:55:25.7 -- not a known variable star
07:00:33.69 -00:05:51.2 -- not a known variable star
07:00:37.09 +02:24:01.4 -- not a known variable star
07:00:51.99 +00:12:01.1 -- not a known variable star
07:01:10.19 +00:00:19.9 -- a known variable star
07:01:18.50 -03:25:51.2 -- not a known variable star
07:01:28.02 -05:15:03.7 -- a known variable star
07:01:34.41 +01:46:03.5 -- not a known variable star
07:01:49.42 -05:35:31.2 -- not a known variable star
07:01:58.09 -02:16:28.4 -- not a known variable star
07:02:06.97 -01:14:09.2 -- not a known variable star
07:02:23.39 -05:08:56.1 -- not a known variable star
07:02:33.02 +02:20:26.1 -- a known variable star
07:02:37.62 -01:54:05.5 -- not a known variable star
07:02:45.30 -04:03:44.7 -- not a known variable star
07:03:00.75 +02:24:11.0 -- a known variable star
07:03:23.58 -00:39:16.9 -- not a known variable star
07:03:30.37 -03:45:39.9 -- not a known variable star
07:03:38.84 -02:31:45.3 -- not a known variable star
07:03:45.85 -02:09:34.0 -- not a known variable star
07:03:46.90 -01:04:51.3 -- not a known variable star
07:03:51.50 +02:00:05.0 -- not a known variable star
07:04:02.03 +02:51:32.4 -- not a known variable star
07:04:10.66 -03:14:37.6 -- not a known variable star
07:04:13.55 +01:59:53.3 -- not a known variable star
07:04:16.64 -03:01:37.2 -- not a known variable star
07:04:19.74 +01:39:45.5 -- not a known variable star
07:04:32.14 +00:11:23.7 -- a known variable star
07:04:32.63 -02:17:38.7 -- a known variable star
07:04:33.73 -04:28:38.5 -- not a known variable star
07:04:34.56 -05:56:28.1 -- a known variable star
07:05:20.36 +02:45:54.9 -- not a known variable star
07:05:20.53 +02:02:06.0 -- not a known variable star
07:05:25.56 -02:12:22.9 -- not a known variable star
07:05:27.95 +00:36:30.6 -- a known variable star
07:05:28.64 -02:00:08.1 -- a known variable star
07:05:38.60 +01:26:03.2 -- not a known variable star
07:05:39.86 +02:28:20.2 -- not a known variable star
07:05:41.30 +02:40:15.0 -- a known variable star
07:05:45.60 -02:32:43.4 -- a known variable star
07:05:46.99 +00:13:15.3 -- a known variable star
07:05:49.20 +02:34:31.7 -- not a known variable star
07:05:52.53 -00:00:59.4 -- not a known variable star
07:05:56.42 -03:14:54.0 -- a known variable star
07:06:18.03 +01:07:23.6 -- not a known variable star
07:06:31.61 +02:05:37.7 -- not a known variable star
07:06:31.68 +02:11:36.3 -- a known variable star
07:06:37.26 +00:11:58.2 -- not a known variable star
07:06:43.05 +01:06:56.7 -- a known variable star
07:06:50.68 -03:05:03.4 -- not a known variable star
07:06:54.08 +02:10:49.3 -- a known variable star
07:06:56.23 +00:23:23.9 -- not a known variable star
07:07:01.92 +00:40:29.5 -- a known variable star
07:07:02.56 -00:42:25.6 -- not a known variable star
07:07:03.67 -02:21:52.0 -- not a known variable star
07:07:06.62 +01:52:36.0 -- not a known variable star
07:07:09.33 -01:15:16.3 -- a known variable star
07:07:11.25 -02:58:19.6 -- not a known variable star
07:07:25.92 -01:50:45.1 -- not a known variable star
07:07:26.07 -02:04:10.2 -- a known variable star
07:07:34.54 -03:27:34.7 -- not a known variable star
07:07:59.09 +02:08:45.2 -- not a known variable star
07:07:59.65 -00:24:51.6 -- not a known variable star
07:08:01.10 -01:31:58.2 -- not a known variable star
07:08:10.19 -03:43:12.7 -- not a known variable star
07:08:11.40 -02:49:43.0 -- not a known variable star
07:08:24.79 +02:46:17.7 -- a known variable star
07:08:31.17 -00:56:08.8 -- not a known variable star
07:08:39.92 -02:15:36.2 -- not a known variable star
07:08:40.99 -00:53:47.0 -- not a known variable star
07:08:41.07 -03:29:16.1 -- not a known variable star
07:08:44.77 -01:27:54.2 -- not a known variable star
07:08:45.27 +00:41:48.2 -- a known variable star
07:08:49.10 -00:04:32.4 -- a known variable star
07:08:51.33 -02:26:19.9 -- not a known variable star
07:08:52.69 -03:55:19.2 -- a known variable star
07:08:52.74 -04:21:47.6 -- not a known variable star
07:08:57.65 -03:05:11.0 -- a known variable star
07:08:58.12 -02:02:47.5 -- not a known variable star
07:09:04.05 -01:41:57.0 -- a known variable star
07:09:08.35 +00:42:47.5 -- not a known variable star
07:09:11.19 -05:50:47.6 -- a known variable star
07:09:12.86 -00:34:11.6 -- not a known variable star
07:09:13.17 +00:26:49.8 -- not a known variable star
07:09:13.71 -02:21:31.0 -- a known variable star
07:09:20.41 +00:20:20.3 -- not a known variable star
07:09:24.18 -01:33:15.7 -- not a known variable star
07:09:28.97 -06:44:34.8 -- not a known variable star
07:09:36.21 +01:42:30.9 -- not a known variable star
07:09:36.61 -03:32:25.0 -- not a known variable star
07:09:37.42 -04:39:36.0 -- a known variable star
07:09:37.99 +02:07:35.5 -- not a known variable star
07:09:40.94 -04:22:45.1 -- not a known variable star
07:09:45.49 -03:50:37.7 -- not a known variable star
07:09:52.27 +00:44:50.4 -- not a known variable star
07:09:56.39 -04:34:53.5 -- not a known variable star
07:10:02.55 -02:31:59.1 -- not a known variable star
07:10:03.22 +01:44:56.9 -- not a known variable star
07:10:10.01 -00:03:44.9 -- not a known variable star
07:10:10.10 +02:03:17.9 -- not a known variable star
07:10:13.28 -01:12:05.9 -- not a known variable star
07:10:20.63 -00:55:59.4 -- not a known variable star
07:10:33.95 -00:34:04.4 -- not a known variable star
07:10:38.42 -00:26:09.2 -- not a known variable star
07:10:41.81 -02:46:24.7 -- not a known variable star
07:10:42.55 -01:49:35.9 -- not a known variable star
07:10:48.74 -00:38:30.1 -- a known variable star
07:10:49.21 -05:23:04.9 -- a known variable star
07:10:55.03 -01:45:30.6 -- not a known variable star
07:10:57.64 +01:38:35.0 -- not a known variable star
07:10:59.09 -03:24:27.9 -- not a known variable star
07:11:08.09 +00:18:35.8 -- not a known variable star
07:11:10.01 +02:18:12.0 -- a known variable star
07:11:19.66 -02:24:42.3 -- not a known variable star
07:11:19.76 -03:51:44.5 -- a known variable star
07:11:20.02 +01:36:58.4 -- not a known variable star
07:11:23.67 -07:04:29.5 -- a known variable star
07:11:29.22 -03:50:43.6 -- a known variable star
07:11:30.81 -04:56:27.0 -- a known variable star
07:11:32.32 +01:26:33.4 -- not a known variable star
07:11:37.83 +01:05:41.3 -- not a known variable star
07:11:38.89 -03:15:42.0 -- not a known variable star
07:11:39.57 -00:20:22.1 -- a known variable star
07:11:43.64 +02:18:05.1 -- not a known variable star
07:11:45.29 -05:40:08.5 -- not a known variable star
07:11:47.40 +01:41:59.3 -- not a known variable star
07:11:49.96 +01:54:46.1 -- not a known variable star
07:11:50.14 +01:30:57.6 -- not a known variable star
07:12:07.31 -02:41:42.0 -- not a known variable star
07:12:17.34 -01:40:18.5 -- not a known variable star
07:12:20.26 +01:25:29.4 -- not a known variable star
07:12:22.74 -04:42:42.9 -- a known variable star
07:12:26.80 +02:04:47.0 -- not a known variable star
07:12:32.05 +00:04:09.4 -- not a known variable star
07:12:47.77 -02:27:16.8 -- not a known variable star
07:12:48.01 -00:27:16.3 -- not a known variable star
07:12:48.06 +02:19:47.3 -- a known variable star
07:12:48.84 +01:20:08.9 -- not a known variable star
07:12:53.04 -00:10:58.7 -- not a known variable star
07:12:55.88 -01:41:31.2 -- a known variable star
07:12:56.17 +02:36:39.4 -- not a known variable star
07:13:03.13 -04:47:14.1 -- not a known variable star
07:13:04.11 -01:16:35.5 -- not a known variable star
07:13:12.01 +00:38:43.6 -- not a known variable star
07:13:14.15 -01:39:24.3 -- not a known variable star
07:13:14.78 -03:26:46.1 -- not a known variable star
07:13:26.54 +00:56:15.8 -- not a known variable star
07:13:29.25 -00:50:57.8 -- not a known variable star
07:13:29.26 -04:08:39.0 -- not a known variable star
07:13:34.27 -04:04:38.4 -- a known variable star
07:13:34.72 -00:26:21.7 -- not a known variable star
07:13:39.24 +00:17:18.6 -- not a known variable star
07:13:40.78 -01:01:26.1 -- not a known variable star
07:13:41.27 -03:39:08.7 -- not a known variable star
07:13:41.67 -03:55:39.1 -- not a known variable star
07:13:50.70 +01:53:52.8 -- not a known variable star
07:14:00.43 -01:15:31.0 -- not a known variable star
07:14:05.46 +00:33:06.9 -- not a known variable star
07:14:06.75 +01:28:20.5 -- not a known variable star
07:14:06.90 -04:20:52.6 -- not a known variable star
07:14:12.32 -04:54:52.4 -- a known variable star
07:14:18.34 -04:09:01.6 -- not a known variable star
07:14:23.75 -00:00:49.6 -- not a known variable star
07:14:25.25 -06:11:44.0 -- a known variable star
07:14:29.95 +01:49:08.2 -- not a known variable star
07:14:33.99 -05:29:12.2 -- not a known variable star
07:14:45.29 -01:22:49.3 -- not a known variable star
07:14:45.36 -06:00:15.5 -- not a known variable star
07:14:46.42 -01:18:37.0 -- not a known variable star
07:14:59.16 -01:45:25.0 -- not a known variable star
07:14:59.81 +01:48:09.3 -- not a known variable star
07:15:05.82 +02:37:23.0 -- not a known variable star
07:15:07.42 -00:40:05.2 -- not a known variable star
07:15:08.46 +00:57:32.7 -- a known variable star
07:15:10.04 +00:21:59.8 -- not a known variable star
07:15:16.33 -04:43:31.4 -- not a known variable star
07:15:25.90 -01:11:23.0 -- not a known variable star
07:15:27.30 -02:29:46.1 -- not a known variable star
07:15:31.16 +00:28:43.2 -- not a known variable star
07:15:35.43 +02:02:01.7 -- not a known variable star
07:15:39.53 -00:49:28.3 -- not a known variable star
07:15:45.85 -02:39:23.4 -- not a known variable star
07:15:46.86 -01:58:00.5 -- not a known variable star
07:15:49.13 -01:44:51.8 -- not a known variable star
07:16:03.06 -00:40:39.8 -- not a known variable star
07:16:03.21 +01:36:13.2 -- not a known variable star
07:16:08.09 -03:04:46.8 -- not a known variable star
07:16:08.79 +00:47:13.0 -- not a known variable star
07:16:14.82 -00:14:34.3 -- not a known variable star
07:16:17.04 +01:00:36.5 -- not a known variable star
07:16:20.97 -00:19:45.3 -- a known variable star
07:16:40.42 -01:23:38.8 -- not a known variable star
07:16:41.81 +02:29:08.8 -- not a known variable star
07:16:46.06 -01:27:55.3 -- not a known variable star
07:16:50.04 -03:31:10.0 -- not a known variable star
07:16:55.49 -04:32:30.0 -- not a known variable star
07:16:58.56 +00:50:26.6 -- not a known variable star
07:17:12.67 +02:26:39.2 -- not a known variable star
07:17:15.35 -02:36:55.8 -- a known variable star
07:17:16.56 -00:42:24.4 -- a known variable star
07:17:17.77 -00:03:13.1 -- not a known variable star
07:17:25.27 +02:31:58.2 -- not a known variable star
07:17:25.66 -04:17:48.9 -- not a known variable star
07:17:28.74 -01:41:40.3 -- not a known variable star
07:17:31.21 +01:05:39.1 -- a known variable star
07:17:32.78 +01:33:25.8 -- a known variable star
07:17:35.03 +01:29:52.9 -- a known variable star
07:17:36.38 +00:20:10.6 -- not a known variable star
07:17:41.20 +00:07:00.0 -- not a known variable star
07:17:41.55 -02:02:57.4 -- a known variable star
07:17:42.14 -00:21:03.7 -- a known variable star
07:17:45.13 -00:17:16.0 -- not a known variable star
07:17:46.83 -02:42:16.0 -- not a known variable star
07:18:00.41 -03:35:48.4 -- not a known variable star
07:18:00.81 +00:09:40.9 -- not a known variable star
07:18:12.82 -01:43:03.6 -- not a known variable star
07:18:14.36 +00:02:43.8 -- not a known variable star
07:18:23.24 +01:03:42.2 -- a known variable star
07:18:29.75 -00:11:36.0 -- not a known variable star
07:18:29.79 +00:52:08.9 -- not a known variable star
07:18:54.14 +01:36:32.4 -- not a known variable star
07:19:06.80 -02:29:52.0 -- not a known variable star
07:19:08.27 -02:01:49.6 -- not a known variable star
07:19:23.66 +00:34:09.9 -- not a known variable star
07:19:24.39 -00:41:30.7 -- a known variable star
07:19:26.37 -01:55:44.5 -- not a known variable star
07:19:27.98 -02:42:29.5 -- not a known variable star
07:19:44.76 -03:04:57.8 -- not a known variable star
07:19:50.40 -02:35:19.8 -- not a known variable star
07:20:03.58 -01:48:50.5 -- not a known variable star
07:20:05.61 -00:29:44.4 -- not a known variable star
07:20:05.65 +01:09:50.0 -- not a known variable star
07:20:20.02 -01:34:22.0 -- not a known variable star
07:20:20.06 -00:44:21.3 -- not a known variable star
07:20:29.07 +02:01:14.6 -- not a known variable star
07:20:31.64 -06:57:28.9 -- not a known variable star
07:20:37.02 -05:27:07.1 -- not a known variable star
07:20:44.53 -05:00:15.3 -- not a known variable star
07:20:55.56 +00:36:26.3 -- not a known variable star
07:21:03.32 +00:12:22.6 -- not a known variable star
07:21:06.40 -03:14:57.8 -- not a known variable star
07:21:16.78 -03:12:16.2 -- a known variable star
07:21:21.93 -00:51:52.0 -- a known variable star
07:21:22.39 -05:02:55.9 -- a known variable star
07:21:23.98 -00:37:27.2 -- not a known variable star
07:21:26.49 -04:48:08.0 -- not a known variable star
07:21:28.67 -04:04:57.4 -- not a known variable star
07:21:31.52 -01:38:19.3 -- not a known variable star
07:21:46.89 -04:08:39.8 -- a known variable star
07:21:59.34 -02:01:00.5 -- not a known variable star
07:22:07.41 -02:10:22.0 -- not a known variable star
07:22:28.38 +00:11:02.8 -- not a known variable star
07:22:32.66 -01:44:04.6 -- not a known variable star
07:22:33.94 -00:33:48.1 -- a known variable star
Found 260 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
348 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 348 (excluding asteroids and hot pixels, 260 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.63468390 -observatory V36
23:20:09.82 -06:26:40.2 Mercury (0.3mag)
02:21:13.25 +13:49:29.5 Venus (-3.9mag)
23:49:44.26 -02:13:42.5 Mars (1.2mag)
07:08:41.05 +22:52:28.8 Jupiter (-2.2mag)
00:24:44.05 +00:21:03.2 Saturn (0.9mag)
03:45:42.68 +19:41:03.5 Uranus (5.8mag)
00:09:31.29 -00:23:43.4 Neptune (7.8mag)
20:33:13.93 -22:52:29.5 Pluto (14.5mag)
15:56:09.36 -25:51:02.7 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 5 23:01 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.63468390:
07:08:46.33 +22:52:16.1 Io (5.7mag)
07:08:53.94 +22:52:02.2 Europa (5.8mag)
07:08:34.41 +22:52:48.8 Ganymede (5.3mag)
07:08:11.82 +22:53:19.0 Callisto (6.5mag)
07:12:24.11 +22:45:00.8 Himalia (15.3mag)
07:08:36.98 +22:52:37.5 Thebe (16.2mag)
07:12:21.71 +23:13:46.0 Elara (17.2mag)
07:06:53.64 +23:37:39.0 Pasiphae (17.3mag)
07:17:12.93 +22:49:24.4 Carme (18.4mag)
00:24:38.51 +00:21:04.9 Titan (8.8mag)
00:24:40.98 +00:21:17.9 Rhea (10.1mag)
00:24:44.75 +00:22:37.1 Iapetus (11.5mag)
00:24:45.60 +00:20:51.8 Hyperion (14.8mag)
00:26:28.31 +00:30:52.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 5 23:02 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.63468390:
14:47:04.96 -08:15:08.1 JWST
16:49:23.91 +45:28:55.0 Chandra
07:51:26.94 -33:28:40.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 5 23:01 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.63468390 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:05.46 -28:13:56.5 14.0mag P/2010 H2 (Vales)
05:00:02.99 -70:09:03.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:33.61 +31:22:32.5 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.72 +09:21:47.4 17.6mag C/2021 G2 (ATLAS)
23:07:19.98 +28:51:58.3 17.0mag C/2022 E2 (ATLAS)
04:17:55.70 +25:45:46.0 15.9mag C/2022 N2 (PANSTARRS)
09:01:51.66 +31:54:20.2 16.1mag C/2022 QE78 (ATLAS)
08:29:59.00 -01:14:21.1 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.80 +17:41:23.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:31.52 -11:39:40.4 17.6mag P/2023 B1 (PANSTARRS)
09:12:52.31 -13:30:46.4 17.5mag C/2023 F3 (ATLAS)
21:43:24.36 +62:22:06.2 17.5mag C/2023 H5 (Lemmon)
19:26:26.69 -03:36:28.8 14.3mag C/2023 R1 (PANSTARRS)
21:42:39.26 +84:36:13.6 17.8mag C/2023 X2 (Lemmon)
06:14:31.11 +63:35:04.1 17.0mag C/2024 A1 (ATLAS)
04:50:55.70 +14:31:49.9 10.4mag C/2024 E1 (Wierzchos)
16:25:08.01 +04:46:06.3 17.4mag C/2024 G6 (ATLAS)
20:17:31.57 +12:40:08.4 14.7mag C/2024 J3 (ATLAS)
03:17:43.06 -23:55:55.9 16.4mag C/2024 T5 (ATLAS)
05:08:39.63 +47:51:01.5 17.7mag C/2025 J1 (Borisov)
14:19:19.79 +37:20:00.5 14.8mag C/2025 L1 (ATLAS)
03:10:17.10 -24:44:27.7 17.8mag C/2025 Q3 (ATLAS)
22:53:25.71 +19:50:13.8 10.1mag C/2025 R3 (PANSTARRS)
12:58:25.03 +02:23:18.4 17.5mag C/2025 Y1 (ATLAS)
01:29:56.18 +04:44:28.0 7.0mag C/2026 A1 (MAPS)
23:30:37.95 +35:13:52.8 14.3mag C/2026 B2 (Sun-Gao)
18:23:40.69 -10:13:15.4 12.4mag 10P/Tempel
15:12:58.30 +04:06:59.3 13.1mag 24P/Schaumasse
11:05:47.47 -01:51:57.2 15.7mag 29P/Schwassmann-Wachmann
17:56:43.69 -09:59:42.8 17.7mag 40P/Vaisala
10:38:53.97 -04:57:12.5 16.7mag 43P/Wolf-Harrington
01:33:27.88 +15:47:10.4 17.1mag 47P/Ashbrook-Jackson
06:53:14.21 +39:05:34.2 17.0mag 63P/Wild
23:16:13.94 -12:39:43.8 15.7mag 65P/Gunn
03:37:31.97 +17:43:00.3 15.8mag 76P/West-Kohoutek-Ikemura
00:43:57.31 +06:16:25.8 14.4mag 78P/Gehrels
22:32:21.90 -12:17:16.5 14.5mag 88P/Howell
01:43:00.97 +17:55:53.3 15.1mag 93P/Lovas
04:36:49.60 +31:43:30.2 16.3mag 123P/West-Hartley
08:17:52.97 +42:55:02.4 16.2mag 124P/Mrkos
02:18:07.88 +13:15:01.7 16.4mag 128P/Shoemaker-Holt
02:28:17.27 +13:14:46.8 17.5mag 131P/Mueller
00:35:35.90 +09:35:16.1 11.3mag 141P/Machholz
00:45:34.58 +01:10:44.3 11.3mag 141P-A/Machholz
23:36:10.74 -02:26:25.9 14.1mag 141P-D/Machholz
01:14:41.30 +02:50:33.7 17.9mag 141P-I/Machholz
00:34:58.72 -06:26:44.9 15.2mag 162P/SidingSpring
10:30:59.85 +31:30:34.8 17.8mag 164P/Christensen
06:18:19.63 +24:31:28.4 17.8mag 198P/ODAS
15:08:47.98 -01:12:10.0 17.4mag 210P/Christensen
21:08:43.72 -13:50:06.1 17.4mag 218P/LINEAR
17:12:34.22 -15:04:45.1 16.2mag 235P/LINEAR
05:13:32.52 +33:51:02.6 16.6mag 240P/NEAT
07:34:10.82 -06:17:37.9 17.6mag 242P/Spahr
15:45:57.25 +06:18:18.3 17.5mag 391P/Kowalski
07:30:54.17 +21:18:40.4 17.6mag 450P/LONEOS
05:21:50.33 +45:36:53.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 5 23:01 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 5 23:01 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
13:10:16.980 +34:24:10.02 AT 2026htp 2026-03-15.74 20.86
-rw-r--r-- 1 apache apache 30K Apr 5 23:01 tns_transients_list.txt
