This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461146.6131,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AG Mon 20260416.1131 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.76,0.05,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
target 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.60,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112566136607539200,2461146.6131,13.70,0.05,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
Gaia DR3 3112566136607539200 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6170-02.9483,2461146.6131,13.65,0.05,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 J106.6170-02.9483 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125982308769563008,2461146.6131,13.61,0.05,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 3125982308769563008 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125981965172191232,2461146.6131,13.64,0.05,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 3125981965172191232 20260416.1131 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.0279-00.2027,2461146.6131,13.71,0.05,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 J101.0279-00.2027 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.6131,13.80,0.05,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
VARIABLE_NAME 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.72,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3599-00.2642,2461146.6131,13.76,0.05,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 J106.3599-00.2642 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.54,0.05,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 20260416.1131 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.71,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126715060248964096,2461146.6131,13.71,0.05,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
Gaia DR3 3126715060248964096 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115379924302540032,2461146.6131,13.65,0.05,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
Gaia DR3 3115379924302540032 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.61,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.49,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.56,0.05,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 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.48,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114377959969588864,2461146.6131,13.66,0.05,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
Gaia DR3 3114377959969588864 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112992712758972672,2461146.6131,13.76,0.05,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 3112992712758972672 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109549935693727616,2461146.6131,13.60,0.05,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
Gaia DR3 3109549935693727616 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.56,0.05,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 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5502+00.5928,2461146.6131,13.55,0.05,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
ATO J106.5502+00.5928 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.63,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5794-01.9625,2461146.6131,13.65,0.05,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 J101.5794-01.9625 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J063732.66+014639.0,2461146.6131,13.56,0.05,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
ZTF J063732.66+014639.0 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0702018-021634,2461146.6131,13.63,0.05,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
GDS_J0702018-021634 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6243-00.5097,2461146.6131,13.66,0.05,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 J107.6243-00.5097 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6031-00.6016,2461146.6131,13.55,0.05,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
ATO J104.6031-00.6016 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114532097757533440,2461146.6131,13.44,0.05,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
Gaia DR3 3114532097757533440 20260416.1131 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.62,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109370371703315584,2461146.6131,13.55,0.05,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
Gaia DR3 3109370371703315584 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.38,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.38,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112411827022500608,2461146.6131,13.46,0.05,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 3112411827022500608 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.49,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.63,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2307-01.9667,2461146.6131,13.39,0.05,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
ATO J108.2307-01.9667 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7822+02.4327,2461146.6131,13.28,0.05,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 J108.7822+02.4327 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112107704678242432,2461146.6131,13.43,0.05,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
Gaia DR3 3112107704678242432 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.48,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114638612946099072,2461146.6131,13.47,0.05,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
Gaia DR3 3114638612946099072 20260416.1131 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.49,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.29,0.05,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
target 20260416.1131 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126166403949008000,2461146.6131,13.45,0.05,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 3126166403949008000 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2154-00.3780,2461146.6131,13.36,0.05,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 J106.2154-00.3780 20260416.1131 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5766+02.5096,2461146.6131,13.41,0.05,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
ATO J106.5766+02.5096 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108441829832289920,2461146.6131,13.34,0.05,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
Gaia DR3 3108441829832289920 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126792202162858240,2461146.6131,13.26,0.05,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 3126792202162858240 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.51,0.05,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 20260416.1131 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107119602680173696,2461146.6131,13.31,0.05,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 3107119602680173696 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.30,0.05,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
target 20260416.1131 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7316-00.9019,2461146.6131,13.43,0.05,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 J107.7316-00.9019 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.8770+00.5215,2461146.6131,13.21,0.05,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
ATO J107.8770+00.5215 20260416.1131 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127775062478075136,2461146.6131,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127775062478075136 20260416.1131 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3139014923171195520,2461146.6131,13.29,0.05,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 3139014923171195520 20260416.1131 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126059132846155520,2461146.6131,13.43,0.05,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
Gaia DR3 3126059132846155520 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.27,0.05,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
target 20260416.1131 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.32,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7677+01.3676,2461146.6131,13.19,0.05,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 J107.7677+01.3676 20260416.1131 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.44,0.05,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 20260416.1131 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111219166142543104,2461146.6131,13.32,0.05,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 3111219166142543104 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.33,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9779+02.9024,2461146.6131,13.31,0.05,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 J103.9779+02.9024 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.8169-04.9476,2461146.6131,13.10,0.05,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 J098.8169-04.9476 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5494+01.3183,2461146.6131,13.18,0.05,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 J104.5494+01.3183 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114074769639625216,2461146.6131,13.22,0.05,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
Gaia DR3 3114074769639625216 20260416.1131 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110606463289588480,2461146.6131,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110606463289588480 20260416.1131 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6668-01.9250,2461146.6131,13.19,0.05,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 J104.6668-01.9250 20260416.1131 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114516910751071104,2461146.6131,13.10,0.05,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
Gaia DR3 3114516910751071104 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127768946444825344,2461146.6131,13.06,0.05,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 3127768946444825344 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2008+01.3366,2461146.6131,13.12,0.05,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 J108.2008+01.3366 20260416.1131 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108382597944368768,2461146.6131,13.03,0.05,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
Gaia DR3 3108382597944368768 20260416.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3116003450473542784,2461146.6131,13.00,0.05,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
Gaia DR3 3116003450473542784 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106052732803548160,2461146.6131,12.94,0.05,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
Gaia DR3 3106052732803548160 20260416.1131 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5480-02.0407,2461146.6131,12.91,0.05,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 J109.5480-02.0407 20260416.1131 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112750781541980032,2461146.6131,12.63,0.05,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
Gaia DR3 3112750781541980032 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114394727522251904,2461146.6131,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114394727522251904 20260416.1131 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.65,0.05,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 20260416.1131 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109841924755441024,2461146.6131,12.79,0.05,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 3109841924755441024 20260416.1131 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108020858619043712,2461146.6131,12.71,0.05,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 3108020858619043712 20260416.1131 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0704125-011414,2461146.6131,12.50,0.05,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
GDS_J0704125-011414 20260416.1131 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4031-00.0467,2461146.6131,12.68,0.05,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 J106.4031-00.0467 20260416.1131 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5386+00.9385,2461146.6131,12.40,0.05,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
ATO J107.5386+00.9385 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112897600704147072,2461146.6131,12.40,0.05,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 3112897600704147072 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109471389332247552,2461146.6131,12.41,0.05,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 3109471389332247552 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7305-03.0153,2461146.6131,12.22,0.05,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 J104.7305-03.0153 20260416.1131 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115543300556247680,2461146.6131,12.31,0.05,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 3115543300556247680 20260416.1131 12.31CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108383555718321408,2461146.6131,12.18,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112151242766551808,2461146.6131,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112151242766551808 20260416.1131 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1090+01.9830,2461146.6131,11.95,0.05,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 J101.1090+01.9830 20260416.1131 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8650-01.8472,2461146.6131,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8650-01.8472 20260416.1131 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110105738822752256,2461146.6131,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110105738822752256 20260416.1131 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6592+00.8198,2461146.6131,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6592+00.8198 20260416.1131 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.0773+01.7811,2461146.6131,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.0773+01.7811 20260416.1131 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461146.6131,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260416.1131 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127472490623297792,2461146.6131,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127472490623297792 20260416.1131 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4102+01.5218,2461146.6131,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4102+01.5218 20260416.1131 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113311193174967552,2461146.6131,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113311193174967552 20260416.1131 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115110269074863232,2461146.6131,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115110269074863232 20260416.1131 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.2107-00.1428,2461146.6131,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J102.2107-00.1428 20260416.1131 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109935795558237568,2461146.6131,11.99,0.05,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 3109935795558237568 20260416.1131 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111562385568206208,2461146.6131,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111562385568206208 20260416.1131 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7633-01.7514,2461146.6131,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.7633-01.7514 20260416.1131 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115211321064418944,2461146.6131,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115211321064418944 20260416.1131 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3280-03.1171,2461146.6131,12.01,0.05,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 J105.3280-03.1171 20260416.1131 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0887-03.0285,2461146.6131,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0887-03.0285 20260416.1131 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12675437,2461146.6131,12.10,0.05,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
NSVS 12675437 20260416.1131 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0704499-021702,2461146.6131,12.31,0.05,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
GDS_J0704499-021702 20260416.1131 12.31CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114610472320210432,2461146.6131,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114610472320210432 20260416.1131 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112803768556485248,2461146.6131,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112803768556485248 20260416.1131 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1131 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126535672355377792,2461146.6131,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126535672355377792 20260416.1131 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112176394095702528,2461146.6131,12.34,0.05,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 3112176394095702528 20260416.1131 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.39,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110294236346089344,2461146.6131,12.31,0.05,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 3110294236346089344 20260416.1131 12.31CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112992025564253184,2461146.6131,12.32,0.05,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 3112992025564253184 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108522231621317504,2461146.6131,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108522231621317504 20260416.1131 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0365+01.8612,2461146.6131,12.52,0.05,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 J109.0365+01.8612 20260416.1131 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112749274012032640,2461146.6131,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112749274012032640 20260416.1131 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111720749603683456,2461146.6131,12.64,0.05,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 3111720749603683456 20260416.1131 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461146.6131,12.48,0.05,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 J100.9580+01.5948 20260416.1131 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112640181842895232,2461146.6131,12.54,0.05,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 3112640181842895232 20260416.1131 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113915787131019392,2461146.6131,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113915787131019392 20260416.1131 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111409553452325120,2461146.6131,12.54,0.05,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 3111409553452325120 20260416.1131 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.69,0.05,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
target 20260416.1131 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110006336102386176,2461146.6131,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110006336102386176 20260416.1131 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1505+01.7467,2461146.6131,12.63,0.05,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
ATO J101.1505+01.7467 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113103071939549184,2461146.6131,12.67,0.05,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
Gaia DR3 3113103071939549184 20260416.1131 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.68,0.05,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
target 20260416.1131 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3130061217731884032,2461146.6131,12.61,0.05,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 3130061217731884032 20260416.1131 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105965733946504448,2461146.6131,12.60,0.05,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
Gaia DR3 3105965733946504448 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113451174747949312,2461146.6131,12.64,0.05,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 3113451174747949312 20260416.1131 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115521344683433984,2461146.6131,12.72,0.05,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 3115521344683433984 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070449.39+023047.8,2461146.6131,12.71,0.05,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
ASASSN-V J070449.39+023047.8 20260416.1131 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115633327372214656,2461146.6131,12.73,0.05,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
Gaia DR3 3115633327372214656 20260416.1131 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2021+00.7657,2461146.6131,12.71,0.05,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
ATO J104.2021+00.7657 20260416.1131 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5787-02.0237,2461146.6131,12.67,0.05,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 J105.5787-02.0237 20260416.1131 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461146.6131,12.71,0.05,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
ATO J106.0676-03.0161 20260416.1131 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127198604847054208,2461146.6131,12.77,0.05,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 3127198604847054208 20260416.1131 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.71,0.05,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 20260416.1131 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461146.6131,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114694099624336256 20260416.1131 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.81,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.73,0.05,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 20260416.1131 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109246607924996352,2461146.6131,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109246607924996352 20260416.1131 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112446977034766080,2461146.6131,12.84,0.05,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
Gaia DR3 3112446977034766080 20260416.1131 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120812576892617856,2461146.6131,12.79,0.05,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 3120812576892617856 20260416.1131 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.82,0.05,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 20260416.1131 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6792-01.8242,2461146.6131,12.77,0.05,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 J107.6792-01.8242 20260416.1131 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126545666739715328,2461146.6131,12.81,0.05,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 3126545666739715328 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109297872654329344,2461146.6131,12.79,0.05,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 3109297872654329344 20260416.1131 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112460441750884224,2461146.6131,12.80,0.05,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
Gaia DR3 3112460441750884224 20260416.1131 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.86,0.05,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
target 20260416.1131 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108544329232043904,2461146.6131,12.91,0.05,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 3108544329232043904 20260416.1131 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110150406482209152,2461146.6131,12.89,0.05,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
Gaia DR3 3110150406482209152 20260416.1131 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112232228669552896,2461146.6131,12.94,0.05,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
Gaia DR3 3112232228669552896 20260416.1131 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3331+02.7602,2461146.6131,12.96,0.05,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 J106.3331+02.7602 20260416.1131 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109325669683966080,2461146.6131,12.98,0.05,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 3109325669683966080 20260416.1131 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125513809436303872,2461146.6131,12.98,0.05,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 3125513809436303872 20260416.1131 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.6982+02.3673,2461146.6131,12.94,0.05,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 J109.6982+02.3673 20260416.1131 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114481137965513216,2461146.6131,12.94,0.05,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
Gaia DR3 3114481137965513216 20260416.1131 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125922381086607360,2461146.6131,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125922381086607360 20260416.1131 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108625826231054976,2461146.6131,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108625826231054976 20260416.1131 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127203655728648192,2461146.6131,12.96,0.05,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 3127203655728648192 20260416.1131 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1615-01.5148,2461146.6131,13.01,0.05,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 J105.1615-01.5148 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.00,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9279-01.2566,2461146.6131,12.99,0.05,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 J104.9279-01.2566 20260416.1131 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MGAB-V1900,2461146.6131,12.95,0.05,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
MGAB-V1900 20260416.1131 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110870517879495168,2461146.6131,13.06,0.05,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 3110870517879495168 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112121349793909632,2461146.6131,13.01,0.05,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 3112121349793909632 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106128697885405184,2461146.6131,12.97,0.05,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
Gaia DR3 3106128697885405184 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7533-02.6015,2461146.6131,13.01,0.05,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 J104.7533-02.6015 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4580+02.5742,2461146.6131,13.02,0.05,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 J106.4580+02.5742 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114789108600839552,2461146.6131,12.99,0.05,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
Gaia DR3 3114789108600839552 20260416.1131 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.07,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461146.6131,13.06,0.05,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 3126271617766100608 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112250233172204032,2461146.6131,12.99,0.05,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
Gaia DR3 3112250233172204032 20260416.1131 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113470691079092224,2461146.6131,13.16,0.05,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 3113470691079092224 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108425204019105664,2461146.6131,13.06,0.05,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 3108425204019105664 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.06,0.05,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
target 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7477+00.2283,2461146.6131,13.06,0.05,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
ATO J102.7477+00.2283 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0154-01.7229,2461146.6131,12.97,0.05,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
ATO J107.0154-01.7229 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461146.6131,13.02,0.05,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
CoRoT 102785122 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109833059942089344,2461146.6131,13.09,0.05,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 3109833059942089344 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6624+00.2039,2461146.6131,13.08,0.05,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 J103.6624+00.2039 20260416.1131 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3377-03.4350,2461146.6131,13.07,0.05,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 J105.3377-03.4350 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114877172608642176,2461146.6131,13.09,0.05,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 3114877172608642176 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114863772310812800,2461146.6131,13.26,0.05,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 3114863772310812800 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127840174182358016,2461146.6131,13.06,0.05,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 3127840174182358016 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110689064100344576,2461146.6131,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110689064100344576 20260416.1131 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113700076693885568,2461146.6131,13.21,0.05,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 3113700076693885568 20260416.1131 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461146.6131,13.04,0.05,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 3108863080225629056 20260416.1131 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070654.13+021046.6,2461146.6131,13.09,0.05,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
ASASSN-V J070654.13+021046.6 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115400608865422336,2461146.6131,13.17,0.05,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 3115400608865422336 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2307+00.9114,2461146.6131,13.27,0.05,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 J104.2307+00.9114 20260416.1131 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126002336198034048,2461146.6131,13.07,0.05,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 3126002336198034048 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126192895306272128,2461146.6131,13.12,0.05,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 3126192895306272128 20260416.1131 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461146.6131,13.10,0.05,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
Gaia DR3 3114460526421262848 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112963713139488384,2461146.6131,13.03,0.05,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
Gaia DR3 3112963713139488384 20260416.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125637852391270784,2461146.6131,13.11,0.05,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 3125637852391270784 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114422142294756608,2461146.6131,13.06,0.05,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 3114422142294756608 20260416.1131 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.11,0.05,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
target 20260416.1131 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
Mean magnitude and position on the discovery images:
2026 04 16.1131 2461146.6131 13.11 07:09:56.82 -00:13:56.2
215.25261 4.01107 galactic Mon Second-epoch detections are separated by 6.1" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3111164843394032000 | 07:09:56.48 -00:14:22.5 (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) SpType: G5 (LAMOST DR5)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3111164843394032000,2461146.6131,13.11,0.05,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
Large-amplitude variable Gaia DR2 3111164843394032000 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0736-03.3663,2461146.6131,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0736-03.3663 20260416.1131 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.09,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115039350573052160,2461146.6131,13.13,0.05,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 3115039350573052160 20260416.1131 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112663683904163584,2461146.6131,13.16,0.05,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 3112663683904163584 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113390186212355840,2461146.6131,13.12,0.05,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 3113390186212355840 20260416.1131 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108798488219749888,2461146.6131,13.15,0.05,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 3108798488219749888 20260416.1131 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2427-02.0482,2461146.6131,13.20,0.05,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
ATO J107.2427-02.0482 20260416.1131 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.09,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113730450702943616,2461146.6131,13.22,0.05,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
Gaia DR3 3113730450702943616 20260416.1131 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063819.72+020600.1,2461146.6131,13.22,0.05,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
ASASSN-V J063819.72+020600.1 20260416.1131 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109836083598822272,2461146.6131,13.12,0.05,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 3109836083598822272 20260416.1131 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109309692404188032,2461146.6131,13.20,0.05,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 3109309692404188032 20260416.1131 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.7941+01.3376,2461146.6131,13.21,0.05,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
ATO J105.7941+01.3376 20260416.1131 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108875037416696192,2461146.6131,13.14,0.05,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
Gaia DR3 3108875037416696192 20260416.1131 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7790+02.9110,2461146.6131,13.25,0.05,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
ATO J101.7790+02.9110 20260416.1131 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.29,0.05,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
target 20260416.1131 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113219246514568576,2461146.6131,13.16,0.05,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 3113219246514568576 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.6375-01.8671,2461146.6131,13.13,0.05,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 J101.6375-01.8671 20260416.1131 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109771762170242304,2461146.6131,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109771762170242304 20260416.1131 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.8062+00.4187,2461146.6131,13.19,0.05,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 J101.8062+00.4187 20260416.1131 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1511+00.9977,2461146.6131,13.28,0.05,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 J101.1511+00.9977 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5773-03.3297,2461146.6131,13.35,0.05,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 J105.5773-03.3297 20260416.1131 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5807+02.8132,2461146.6131,13.34,0.05,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 J104.5807+02.8132 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.15,0.05,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
target 20260416.1131 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.21,0.05,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 20260416.1131 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112948251257159808,2461146.6131,13.31,0.05,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 3112948251257159808 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112684467244763008,2461146.6131,13.30,0.05,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 3112684467244763008 20260416.1131 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.34,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070938.64-000118.1,2461146.6131,13.34,0.05,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
ZTF J070938.64-000118.1 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114315665764303488,2461146.6131,13.28,0.05,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 3114315665764303488 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.35,0.05,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 20260416.1131 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115387616581722368,2461146.6131,13.32,0.05,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 3115387616581722368 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5414-00.0643,2461146.6131,13.19,0.05,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 J107.5414-00.0643 20260416.1131 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.7297-02.0389,2461146.6131,13.34,0.05,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 J105.7297-02.0389 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106318947754976512,2461146.6131,13.32,0.05,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 3106318947754976512 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126439671246457344,2461146.6131,13.32,0.05,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 3126439671246457344 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4148+01.7142,2461146.6131,13.36,0.05,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 J107.4148+01.7142 20260416.1131 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461146.6131,13.25,0.05,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
ATO J101.9913-01.3476 20260416.1131 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127770183395674880,2461146.6131,13.41,0.05,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 3127770183395674880 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7913+00.9506,2461146.6131,13.38,0.05,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 J103.7913+00.9506 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.26,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108459460677899520,2461146.6131,13.34,0.05,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
Gaia DR3 3108459460677899520 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115699847824168192,2461146.6131,13.33,0.05,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 3115699847824168192 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4280-01.9828,2461146.6131,13.28,0.05,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 J103.4280-01.9828 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8938-01.1359,2461146.6131,13.46,0.05,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 J108.8938-01.1359 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.28,0.05,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
target 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17329,2461146.6131,13.28,0.05,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
NSV 17329 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113244500922158464,2461146.6131,13.31,0.05,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 3113244500922158464 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9614-02.2114,2461146.6131,13.37,0.05,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 J103.9614-02.2114 20260416.1131 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.4872+00.7123,2461146.6131,13.51,0.05,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 J109.4872+00.7123 20260416.1131 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2271-02.9865,2461146.6131,13.41,0.05,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
ATO J103.2271-02.9865 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3118874855148856448,2461146.6131,13.25,0.05,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 3118874855148856448 20260416.1131 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.46,0.05,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 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112456559100452352,2461146.6131,13.29,0.05,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 3112456559100452352 20260416.1131 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.46,0.05,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 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3335+01.2242,2461146.6131,13.39,0.05,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
ATO J102.3335+01.2242 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.1917+01.0934,2461146.6131,13.54,0.05,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 J103.1917+01.0934 20260416.1131 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0837+00.8377,2461146.6131,13.28,0.05,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 J106.0837+00.8377 20260416.1131 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5128+02.1105,2461146.6131,13.41,0.05,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
ATO J103.5128+02.1105 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461146.6131,13.51,0.05,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 J104.6381-01.6369 20260416.1131 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.59,0.05,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 20260416.1131 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127148924965286656,2461146.6131,13.42,0.05,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
Gaia DR3 3127148924965286656 20260416.1131 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126257835210554368,2461146.6131,13.44,0.05,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
Gaia DR3 3126257835210554368 20260416.1131 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111221124647549312,2461146.6131,13.44,0.05,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
Gaia DR3 3111221124647549312 20260416.1131 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.52,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109579137170282880,2461146.6131,13.46,0.05,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 3109579137170282880 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064630.95+010809.2,2461146.6131,13.37,0.05,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
ASASSN-V J064630.95+010809.2 20260416.1131 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1227+02.6856,2461146.6131,13.60,0.05,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 J105.1227+02.6856 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111277818210788480,2461146.6131,13.47,0.05,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
Gaia DR3 3111277818210788480 20260416.1131 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115440431801220224,2461146.6131,13.39,0.05,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 3115440431801220224 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.4908+03.0785,2461146.6131,13.62,0.05,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 J097.4908+03.0785 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112466252847525120,2461146.6131,13.52,0.05,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
Gaia DR3 3112466252847525120 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2327-02.3822,2461146.6131,13.47,0.05,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 J103.2327-02.3822 20260416.1131 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.56,0.05,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 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.8143+01.9184,2461146.6131,13.59,0.05,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 J103.8143+01.9184 20260416.1131 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2609-00.5555,2461146.6131,13.35,0.05,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 J108.2609-00.5555 20260416.1131 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114107102153036288,2461146.6131,13.49,0.05,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
Gaia DR3 3114107102153036288 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9442+01.1817,2461146.6131,13.44,0.05,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 J107.9442+01.1817 20260416.1131 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112629495964710016,2461146.6131,13.50,0.05,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
Gaia DR3 3112629495964710016 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125817485103519104,2461146.6131,13.50,0.05,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
Gaia DR3 3125817485103519104 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115443210639267200,2461146.6131,13.62,0.05,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
Gaia DR3 3115443210639267200 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.46,0.05,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 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1551+02.0656,2461146.6131,13.62,0.05,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 J106.1551+02.0656 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9413-02.3695,2461146.6131,13.52,0.05,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 J104.9413-02.3695 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126164415382271232,2461146.6131,13.36,0.05,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 3126164415382271232 20260416.1131 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3834+02.0519,2461146.6131,13.55,0.05,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
ATO J102.3834+02.0519 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.66,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3694-00.1977,2461146.6131,13.65,0.05,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 J101.3694-00.1977 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0817+01.8035,2461146.6131,13.51,0.05,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 J105.0817+01.8035 20260416.1131 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.56,0.05,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 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0982+00.9925,2461146.6131,13.56,0.05,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 J106.0982+00.9925 20260416.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112428422775934592,2461146.6131,13.59,0.05,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
Gaia DR3 3112428422775934592 20260416.1131 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.52,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.70,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.6107+00.4430,2461146.6131,13.64,0.05,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
ATO J109.6107+00.4430 20260416.1131 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.76,0.05,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
target 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.8298+02.7686,2461146.6131,13.61,0.05,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
ATO J101.8298+02.7686 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.60,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109432425389948800,2461146.6131,13.64,0.05,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 3109432425389948800 20260416.1131 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.79,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7795+01.7786,2461146.6131,13.67,0.05,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 J101.7795+01.7786 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115119099527484928,2461146.6131,13.62,0.05,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
Gaia DR3 3115119099527484928 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111212500353397632,2461146.6131,13.49,0.05,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
Gaia DR3 3111212500353397632 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7025+01.8262,2461146.6131,13.58,0.05,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 J108.7025+01.8262 20260416.1131 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.66,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113839096195943168,2461146.6131,13.59,0.05,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
Gaia DR3 3113839096195943168 20260416.1131 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.66,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.71,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.61,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2675+01.5073,2461146.6131,13.60,0.05,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 J106.2675+01.5073 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114271513501056128,2461146.6131,13.65,0.05,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
Gaia DR3 3114271513501056128 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.65,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.71,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125763471594615168,2461146.6131,13.54,0.05,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 3125763471594615168 20260416.1131 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5413+01.6888,2461146.6131,13.65,0.05,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 J103.5413+01.6888 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.62,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115074775463019904,2461146.6131,13.69,0.05,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 3115074775463019904 20260416.1131 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
Mean magnitude and position on the discovery images:
2026 04 16.1131 2461146.6131 13.58 06:49:40.20 -01:56:05.1
214.45263 -1.27528 galactic Mon Second-epoch detections are separated by 5.9" and 10.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3106290605273457792 | 06:49:38.04 -01:55:53.1 (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) SpType: F7IV 2012A&A...543A.125G CoRoT 102955078 J-Ks=0.426+/-0.042 (G)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3106290605273457792,2461146.6131,13.58,0.05,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
Large-amplitude variable Gaia DR2 3106290605273457792 20260416.1131 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.60,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7594+03.1305,2461146.6131,13.55,0.05,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
ATO J101.7594+03.1305 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8218-02.7605,2461146.6131,13.57,0.05,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 J106.8218-02.7605 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.65,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9676+01.9141,2461146.6131,13.72,0.05,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 J107.9676+01.9141 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9128+01.5377,2461146.6131,13.82,0.05,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
ATO J103.9128+01.5377 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114816665109744384,2461146.6131,13.73,0.05,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 3114816665109744384 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.46,0.05,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 20260416.1131 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.6463+01.1226,2461146.6131,13.61,0.05,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
ATO J108.6463+01.1226 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.64,0.05,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 20260416.1131 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9328-01.9238,2461146.6131,13.69,0.05,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 J102.9328-01.9238 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.80,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.67,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.3983+01.0125,2461146.6131,13.72,0.05,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 J103.3983+01.0125 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.73,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112162787639018112,2461146.6131,13.65,0.05,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
Gaia DR3 3112162787639018112 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.66,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.79,0.05,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
target 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0987+01.4219,2461146.6131,13.72,0.05,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 J107.0987+01.4219 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.60,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114531616721622912,2461146.6131,13.54,0.05,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 3114531616721622912 20260416.1131 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106251121632857344,2461146.6131,13.67,0.05,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
Gaia DR3 3106251121632857344 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.62,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.58,0.05,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 20260416.1131 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5026-02.1387,2461146.6131,13.63,0.05,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
ATO J105.5026-02.1387 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110981465473380096,2461146.6131,13.62,0.05,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
Gaia DR3 3110981465473380096 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.77,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.9401-02.6616,2461146.6131,13.52,0.05,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 J108.9401-02.6616 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111665464782829952,2461146.6131,13.73,0.05,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 3111665464782829952 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070541.48+024011.8,2461146.6131,13.70,0.05,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
ASASSN-V J070541.48+024011.8 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.73,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5858-01.9330,2461146.6131,13.72,0.05,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 J104.5858-01.9330 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104926523657379840,2461146.6131,13.62,0.05,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
Gaia DR3 3104926523657379840 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.82,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4678+01.8985,2461146.6131,13.61,0.05,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
ATO J108.4678+01.8985 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.1024+00.8457,2461146.6131,13.71,0.05,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 J104.1024+00.8457 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.74,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7809+00.7040,2461146.6131,13.69,0.05,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 J099.7809+00.7040 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071507.71+005721.0,2461146.6131,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071507.71+005721.0 20260416.1131 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9170-00.1509,2461146.6131,13.72,0.05,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 J107.9170-00.1509 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.0070-01.1157,2461146.6131,13.72,0.05,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 J100.0070-01.1157 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.64,0.05,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 20260416.1131 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.68,0.05,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 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108959734168465664,2461146.6131,13.66,0.05,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
Gaia DR3 3108959734168465664 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1131 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126400290687615232,2461146.6131,13.76,0.05,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 3126400290687615232 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0656207-024907,2461146.6131,13.72,0.05,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
GDS_J0656207-024907 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,13.76,0.05,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
target 20260416.1131 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6212+00.7113,2461146.6131,13.68,0.05,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 J104.6212+00.7113 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.4896+01.8732,2461146.6131,13.88,0.05,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 J101.4896+01.8732 20260416.1131 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3653-03.1347,2461146.6131,13.79,0.05,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 J102.3653-03.1347 20260416.1131 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461146.6131,10.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Mon 20260416.1131 10.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0801 Mon,2461146.6131,11.90,0.05,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
V0801 Mon 20260416.1131 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0641591-011108,2461146.6131,12.76,0.05,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
GDS_J0641591-011108 20260416.1131 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6131,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1131 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461146.6131,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BM Mon 20260416.1131 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.4806-04.5084,2461146.6131,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.4806-04.5084 20260416.1131 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.1298-04.0984,2461146.6131,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.1298-04.0984 20260416.1131 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J070529-0200.2,2461146.6131,11.72,0.05,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
ASAS J070529-0200.2 20260416.1131 11.72CV 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
## 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: 2461146.61351441 16.04.2026 02:43:17.645 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
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: 9 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): 37080
Objects passed selection criteria: 37039
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: 34514
Average stars matched: 33263.5 (96.3768 %)
Memory usage VmPeak: 136940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:35:13 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: 2461146.61351441 16.04.2026 02:43:17.645 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1244
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: 341 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): 258241
Objects passed selection criteria: 257565
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: 240423
Average stars matched: 229804 (95.5834 %)
Memory usage VmPeak: 2475120 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:44:07 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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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: 2461146.61270135
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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.4'x636.3' 15.7(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.98"/pix along the Y axis
Image center: 06:51:28.578 -01:58:41.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:28.578 -01:58:41.71
Angular distance between the image centers 0.0659 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:31.553 -01:59:24.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:31.553 -01:59:24.34
Angular distance between the image centers 0.0502 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 06:51:28.578 -01:58:41.71
Second-epoch second image center 06:51:31.553 -01:59:24.34
Angular distance between the image centers 0.01714 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.qYazZtjCqg
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.lrYiMrLw2Z
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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits &> /tmp/tmp.UcmEYcs53J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.Topr1s9078
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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 54 candidate transients before the final filtering. (Hard limit: 8000)
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
2.3 pix fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
14.9 mag. fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (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.qYazZtjCqg (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-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.lrYiMrLw2Z (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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...
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.UcmEYcs53J (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3384, passed=32883
Got 32883 stars (including 29468 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 32883 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 410 to 470 (Dec -7.9 to 3.8)
Done reading UCAC5 zone files...
Matched 667 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 623 matched stars entering correct_measured_positions(), 564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 615 matched stars entering correct_measured_positions(), 19414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.90"
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 410 to 470 (Dec -7.9 to 3.8)
Done reading UCAC5 zone files...
Matched 720 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 690 matched stars entering correct_measured_positions(), 19436 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.84"
Accuracy estimation diagnostic: 688 matched stars entering correct_measured_positions(), 21728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.90"
Excluding outliers - 688 stars left (next iteration limit 676)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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.Topr1s9078 (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3438, passed=32945
Got 32945 stars (including 29481 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 32945 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 30136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 30136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 30136 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 933 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_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52866.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52522_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 52522_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (116.4") between the two second-epoch detections
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Considering the candidate 52523_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 52523_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (64.3") between the two second-epoch detections
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Considering the candidate 52524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 52524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:41.24 -01:19:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.181 3112125266804129152 103.92138591720 -01.32254753295 11.8545 11.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52705_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 52705_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:06.46 +01:45:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 52866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 52951_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 52951_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:31.30 +01:05:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 4.720 3111748198735945984 109.38142228257 +01.09484165755 10.3371 8.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:01.83 -05:27:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53295_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53295_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (52.3") between the two second-epoch detections
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Considering the candidate 53385_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53385_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:09.68 -02:35:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.230 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.0") between the two second-epoch detections
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Considering the candidate 53441_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53441_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:45.36 +00:41:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.179 3114302329885570688 107.18869775869 +00.69614230443 11.9358 11.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:32:20.00 +00:04:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53469_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53469_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:36.22 -02:12:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53480_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53480_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:44.27 -02:34:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.954 3106104714788050432 101.93458736101 -02.57691600924 12.0161 11.7182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53491_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53491_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 53493_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53493_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:06.84 -01:21:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.199 3112286340957262976 103.52816984743 -01.35915272705 11.9522 11.5119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53498_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53498_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:01.95 -01:58:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.964 3106243184533303808 102.50792666588 -01.97042486853 12.1654 12.0227 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 53508_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53508_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:24.54 -02:50:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53510_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53510_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (107.2") between the two second-epoch detections
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Considering the candidate 53513_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53513_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:07.16 -03:17:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.465 3102824905960778368 103.27958426428 -03.28844352308 11.9801 11.6215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:23.89 -02:34:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:29.40 -02:44:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:12.21 -01:48:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53518_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53518_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:37.78 +00:43:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.167 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:09.41 -03:05:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53540_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53540_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:54.62 -02:39:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.475 3106089046747361664 102.22766189689 -02.66193005359 12.0134 11.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53560_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53560_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:02.66 -03:31:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (138.8") between the two second-epoch detections
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Considering the candidate 53570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:17.65 -02:07:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:55.88 -01:31:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53577_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53577_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:58.47 +00:32:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.783 3113027519173665152 105.74308942653 +00.53505361358 12.0753 11.6712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53584_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53584_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:37.69 -03:25:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.456 3102798414602508800 103.15670783379 -03.41972905986 12.0065 11.5164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53585_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53585_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:31.48 -02:06:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.403 3106202163304545664 101.88109323703 -02.10510799966 12.0383 11.5927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:59.65 -05:32:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:09.36 -03:38:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 4.096 3105417661758290432 102.53901700476 -03.64244311062 11.8268 10.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53594_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53594_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (92.7") between the two second-epoch detections
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Considering the candidate 53600_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53600_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (116.1") between the two second-epoch detections
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Considering the candidate 53601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:20.59 -01:09:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:45.66 -03:30:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53610_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53610_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:49.76 -02:12:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.396 3108991693024899200 104.45688285094 -02.20724010665 12.1096 11.7006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:13.00 -03:05:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53626_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53626_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:36:08.17 -03:23:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.843 3104921713294147712 099.03374623654 -03.39027966343 12.0405 11.6214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:46.09 -04:29:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:04.27 -01:34:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.013 3117588735782136576 097.01746922738 -01.58087359653 12.1397 11.9142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53640_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53640_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:34.72 -02:27:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.404 3108229971989266176 109.39442585996 -02.46105686823 12.1728 11.6888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53641_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53641_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:58.59 +00:09:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 4.072 3119546897273221760 100.24313355558 +00.16278864126 12.2670 11.7884 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#
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Considering the candidate 53644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:36.00 -02:03:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:24.94 -01:42:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.431 3118286685148803584 095.60386669068 -01.70956087597 12.2053 11.8886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53650_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53650_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:50.09 -02:30:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.230 3106150722477720192 101.70886789962 -02.50965411492 11.8322 11.0362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53652_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53652_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:48.00 -02:24:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.886 3106122379993182208 102.44990402444 -02.41415379239 12.1563 11.9525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53658_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53658_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:44.71 -03:05:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.877 3105651789015105280 100.43616043331 -03.08778244356 12.1264 11.8425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:07.53 -03:08:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.241 3106389453941350272 099.78120063965 -03.13787545398 12.0397 11.5495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 53664_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 53664_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:41.83 -02:39:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.898 3105950753100683392 103.42406823688 -02.66555116647 12.0807 11.7106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (300.8") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
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 ####
07:09:13.73 -02:21:30.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Image size: 941.4'x636.3' 15.7(deg)x10.6(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.98"/pix along the Y axis
Image center: 06:51:28.578 -01:58:41.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:28.578 -01:58:41.71
Angular distance between the image centers 0.0659 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
Image size: 941.2'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:31.553 -01:59:24.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:31.553 -01:59:24.34
Angular distance between the image centers 0.0502 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 06:51:28.578 -01:58:41.71
Second-epoch second image center 06:51:31.553 -01:59:24.34
Angular distance between the image centers 0.01714 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.o4ORKL7XL7
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.uN6waRtD6U
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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits &> /tmp/tmp.4kbvQY9o9N
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.GtzCEtEEGt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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 1160 candidate transients before the final filtering. (Hard limit: 8000)
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
2.2 pix fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
14.1 mag. fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (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.o4ORKL7XL7 (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-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.uN6waRtD6U (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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...
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.4kbvQY9o9N (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=35004, passed=227661
Got 227661 stars (including 192364 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 227661 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 410 to 470 (Dec -7.9 to 3.8)
Done reading UCAC5 zone files...
Matched 662 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 624 matched stars entering correct_measured_positions(), 564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 620 matched stars entering correct_measured_positions(), 150469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
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 410 to 470 (Dec -7.9 to 3.8)
Done reading UCAC5 zone files...
Matched 713 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 687 matched stars entering correct_measured_positions(), 150488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.47"
Accuracy estimation diagnostic: 686 matched stars entering correct_measured_positions(), 164156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.49"
Excluding outliers - 686 stars left (next iteration limit 682)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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.GtzCEtEEGt (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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=69, blended=35009, passed=226269
Got 226269 stars (including 190965 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 226269 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 3.8)
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...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 214938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 214940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 214935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 933 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_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/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_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-42-07_20.00sec_-4.90C_LIGHTs_0029.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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_2026-04-15_CI_Mon-02-Q1b1x1_214632_TTUQ1b1x1_31102_Xh5C4trA/wcs_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030.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
Adding exclusion_list_gaiadr2.txt__out184359.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out293507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288776.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288924.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out291896.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out293334.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out294442.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out295682.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296302.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296514.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296635.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296896.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out297073.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out297108.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out297138.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out297285.dat to exclusion_list_apass.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__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288533.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__out288553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290864.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out291172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292244.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out292303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293237.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293440.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out293476.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out293511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293534.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out293677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293721.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out293728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293931.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out293970.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294036.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294066.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294190.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294415.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294532.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294776.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out294838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294935.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out295104.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out295165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295422.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out295621.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out295778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295798.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out295838.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296228.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296239.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296273.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296614.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296626.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296661.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296726.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296741.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296806.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out296988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297021.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out297057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78004.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 530s
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: 301s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288464_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288464_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288484_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288484_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288487_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288487_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:09.04 -00:45:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.160 3110233174792816640 109.28674857691 -00.75722981554 14.3641 13.6470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288498_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288498_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288499_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288499_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288511_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288511_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:41.00 +02:06:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.344 3115529457883476480 105.92012447301 +02.10017693865 14.7972 14.2707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288515_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288515_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:48.97 +00:23:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.365 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288518_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:54.03 -01:49:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.646 3112042077576999168 104.22356995745 -01.83123818809 14.1658 13.0980 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 288520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288528_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288528_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:10.77 +01:26:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.634 3114639540659097472 106.29399905678 +01.44949781374 14.5850 14.0730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288530_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288530_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:25.62 -01:05:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 288531_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288531_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:28.51 +03:01:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.408 3127842063967195392 103.61773770839 +03.02715183520 14.0948 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (53.1") between the two second-epoch detections
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Considering the candidate 288533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:20.88 -01:02:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.488 3109380576544706816 107.83630899170 -01.04581544531 14.1534 13.4288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288542_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288542_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288543_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288543_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:02.38 +01:44:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.829 3111891654941507328 110.25911523847 +01.74796682070 14.3602 13.7648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288551_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288551_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:37.89 -00:44:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.349 3112589329430860032 105.90782726838 -00.74461208084 14.6240 14.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288554_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288554_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288561_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288561_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:41.85 -03:32:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.748 3105572418019801216 100.67337610879 -03.54957724967 14.2149 13.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288563_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288563_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.6") between the two second-epoch detections
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Considering the candidate 288573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:06.37 +01:36:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.184 3126133457258796672 102.27573289503 +01.60933180268 14.4170 13.5158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288578_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288578_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:48.77 -02:23:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288581_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288581_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (55.4") between the two second-epoch detections
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Considering the candidate 288588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:02.63 +02:18:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.772 3115548836776134400 106.51000497315 +02.30917447577 14.4001 13.6944 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 288590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288591_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288591_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 288596_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288596_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288597_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288597_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288598_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288598_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:28.76 +01:59:25.9 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 288601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288605_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288605_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (114.6") between the two second-epoch detections
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Considering the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288609_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288609_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:16.33 +01:34:59.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 288612_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288612_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 288615_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288615_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:23.28 -01:51:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.051 3109218054983316864 107.34624767648 -01.85647621958 14.4780 14.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (163.1") between the two second-epoch detections
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Considering the candidate 288620_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288620_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288624_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288624_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288629_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288629_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288631_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288631_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.9") between the two second-epoch detections
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Considering the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288633_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:39.00 +01:25:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.720 3111854512064229248 109.66176333397 +01.41719698700 14.3051 13.6471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288635_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288635_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:24.45 +01:55:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.088 3115476131569810816 105.35103771417 +01.91836098658 14.6331 14.0676 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 288639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288641_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288641_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (53.9") between the two second-epoch detections
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Considering the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288645_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288645_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288649_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288649_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:37.42 -00:06:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.445 3120042025398927488 097.65580090068 -00.11030825243 13.6865 12.4305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288653_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288653_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:34.11 +02:39:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.693 3115208847163215744 107.39138097421 +02.66232076214 14.4352 13.8570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288655_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288655_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:55.36 -00:50:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.816 3119191896752908416 098.48022964590 -00.84694637738 14.1601 13.5383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288666_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288666_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:20.67 +00:20:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.610 3111272355017234048 107.33495773964 +00.33866760416 14.5212 13.9900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288668_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288668_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 288670_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288670_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 288673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:04.98 +00:16:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.471 3113556418627340160 102.52022265106 +00.27669937215 14.2226 13.2762 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 288679_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288679_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:37.20 +02:49:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.314 3127225680322194688 101.65463985773 +02.82944951537 14.6064 13.9592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288682_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288682_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (120.8") between the two second-epoch detections
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Considering the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288685_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:19.17 +01:07:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288688_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288688_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288690_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288690_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288695_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288695_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288698_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:54.19 +01:18:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.420 3111805240199035392 108.72485727634 +01.31366121221 14.1725 13.6944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:43.70 +01:36:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.618 3114123663546924160 103.93110009191 +01.60225901579 14.3268 13.7833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288713_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:12.00 +02:10:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.783 3115099922494413056 107.79918397278 +02.17786501757 14.3074 13.9252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288714_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288714_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (210.9") between the two second-epoch detections
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Considering the candidate 288715_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288715_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288723_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288723_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:24.58 +01:57:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288725_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288725_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:01.30 +00:39:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.907 3113078680823551744 105.50499158530 +00.65039666052 14.2419 13.4343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:37.66 +00:58:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.242 3111590801071481472 110.15602441583 +00.98028564100 14.2742 13.7324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (78.4") between the two second-epoch detections
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Considering the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288744_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288744_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (87.1") between the two second-epoch detections
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Considering the candidate 288745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288746_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288746_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (211.9") between the two second-epoch detections
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Considering the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288751_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288751_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:43.08 +00:23:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.162 3111277096660973824 107.67871891033 +00.38567537619 14.4401 13.9214 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 288755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288759_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:01.86 +00:37:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.136 3114297386383809152 107.00691226902 +00.62360276551 14.1345 13.6096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:56.30 +01:25:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (58.8") between the two second-epoch detections
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Considering the candidate 288763_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288763_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288769_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288769_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:22.22 +02:56:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.157 3127795678321354752 104.59130772371 +02.93545583723 13.8170 12.7648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288773_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288773_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288776_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288776_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:25.10 -01:21:39.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 288782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (71.7") between the two second-epoch detections
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Considering the candidate 288786_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288786_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:40.17 +01:10:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.846 3114427193177580160 108.16636845873 +01.17655047980 14.2983 13.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288787_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:43.44 -01:49:09.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
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Considering the candidate 288790_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288790_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:29.46 +02:24:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.471 3126435960394797184 101.37336664869 +02.40875830565 14.5497 14.0450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288795_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288795_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:16.32 +00:30:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.169 3111466796776706048 110.06738012824 +00.50298598311 14.1510 13.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (48.2") between the two second-epoch detections
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Considering the candidate 288806_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288806_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 288807_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288807_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288808_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288812_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288812_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288816_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288816_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:07.39 +02:20:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288824_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288824_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:39.35 -00:12:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.557 3113246871743868672 102.66307355868 -00.20118987143 14.2112 13.6471 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 288829_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288829_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:11.90 +00:14:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.063 3125505739198071040 101.29884931989 +00.24208721242 14.2269 13.7415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288831_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288831_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (372.6") between the two second-epoch detections
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Considering the candidate 288833_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288833_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288839_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288839_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288850_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288850_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:58.56 +02:26:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.934 3115732145978372352 104.49313066148 +02.43383706770 14.4271 13.9121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288853_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288853_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288854_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288854_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:44.64 -00:17:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.406 3110286986441368320 109.43505872538 -00.28448479516 14.2038 13.5252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288855_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288855_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 288858_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288858_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (43.8") between the two second-epoch detections
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Considering the candidate 288860_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288860_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:52.05 +01:20:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.633 3115367211199527296 105.46601850960 +01.33474391831 14.0347 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:19.47 +01:29:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (93.8") between the two second-epoch detections
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Considering the candidate 288864_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288864_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 288866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:31.82 +02:28:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.460 3124048439614249984 097.38157476050 +02.46605700743 14.0781 13.3972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:59.08 +00:18:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:26.91 +01:34:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288873_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288873_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (178.5") between the two second-epoch detections
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Considering the candidate 288876_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288876_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:30.51 -00:42:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288877_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288877_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:56.30 -02:14:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.838 3108251893502200192 109.48443486195 -02.24351641744 13.9286 13.2644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:01.15 +01:29:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288881_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288881_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288882_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288882_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:37.27 -01:55:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.413 3109776641251247872 109.90386857553 -01.93132100694 14.1354 13.2251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288888_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288888_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288889_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288889_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288890_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288890_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:14.36 +03:05:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288891_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288891_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:41.74 -00:46:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 2.512 3109621025991824896 106.67343921714 -00.76995325981 14.2122 13.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:12.05 +00:06:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.822 3111242152807323776 107.29916214691 +00.09921903946 14.1644 13.3350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288897_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288897_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288900_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288900_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288905_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288905_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.5") between the two second-epoch detections
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Considering the candidate 288906_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288906_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288907_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288907_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:21.73 -00:32:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288910_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288910_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:49.41 +00:06:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.127 3111426252285597568 109.70508366275 +00.11378042853 13.9689 13.2747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:29.69 +02:34:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.918 3126833330769308416 100.87365709262 +02.58277529869 14.0707 13.1486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (146.2") between the two second-epoch detections
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Considering the candidate 288914_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288914_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288915_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288915_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:48.73 +02:15:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.469 3115547153148988544 106.45228695400 +02.26456698191 14.1530 13.6908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288919_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288919_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:36.85 -01:03:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.570 3112415331715647360 103.90268016435 -01.05696012761 13.7754 12.6606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288920_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288920_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288921_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288921_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:35.98 -00:42:22.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 288924_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288924_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:47.55 -00:37:50.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 288929_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288929_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:09.51 +00:44:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.920 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288938_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288938_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288939_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288939_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288941_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288941_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:02.65 -00:20:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.147 3111162850532142080 107.51058836653 -00.34919786351 14.0278 13.1867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288943_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288943_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (103.0") between the two second-epoch detections
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Considering the candidate 288945_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288945_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:47.15 +01:14:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.306 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288947_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288947_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:33.31 +01:48:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 2.545 3126155688009474560 102.13822007435 +01.81525048863 14.2217 13.7290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288951_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288951_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:24.65 +00:38:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.757 3123296545457558656 096.10188687507 +00.63271722889 13.9067 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:36.14 +00:07:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.839 3111112547874786304 108.89966901416 +00.12247911678 14.0533 13.6115 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 288955_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288955_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288957_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288957_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288960_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288960_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.8") between the two second-epoch detections
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Considering the candidate 288965_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288965_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:52.73 +00:01:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.570 3113451380906335232 102.21892944748 +00.02016379598 13.9266 13.1774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288969_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288969_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288970_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288970_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:20.91 +02:44:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288973_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288973_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:10.30 -00:32:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288975_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288975_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:48.66 +00:56:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.306 3111405013668859008 108.45185043368 +00.94629483095 13.7342 13.0393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288977_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288977_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:45.42 +02:45:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.672 3115814952948194304 105.43830860513 +02.76128401817 14.0265 13.2167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288978_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288978_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:52.10 +02:28:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288979_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288979_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:02.22 +02:51:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.488 3115831273824265472 106.00843534485 +02.85827937479 13.7022 13.2566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288981_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288981_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:05.61 +02:16:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288982_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288982_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:06.44 +01:59:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.071 3115434315767919232 105.77630847336 +01.98443851407 13.7473 12.9613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288984_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288984_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288985_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 288985_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 288986_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288986_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:37.13 +01:52:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288989_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288989_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:24.54 -00:41:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.759 3110211017060985344 109.85146786228 -00.69283054811 14.0230 13.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288999_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 288999_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (123.3") between the two second-epoch detections
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Considering the candidate 289002_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289002_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (71.9") between the two second-epoch detections
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Considering the candidate 289004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 289006_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289006_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:02.66 +01:09:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289007_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289007_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (223.6") between the two second-epoch detections
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Considering the candidate 289009_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289009_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:32.62 +02:36:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.397 3126456095201209216 101.88575045793 +02.60695487626 13.6538 12.6852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289011_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289011_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:53.75 +01:01:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289012_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289012_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (75.7") between the two second-epoch detections
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Considering the candidate 289014_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289014_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.0") between the two second-epoch detections
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Considering the candidate 289019_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289019_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (351.7") between the two second-epoch detections
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Considering the candidate 289022_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289022_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (42.1") between the two second-epoch detections
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Considering the candidate 289024_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289024_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:42.79 -00:01:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.570 3111083720054378880 108.92746619878 -00.03013289273 13.7345 13.0456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:29.78 +02:30:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.092 3115754509872056192 104.87304614867 +02.50886577454 13.8045 13.2690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289029_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289029_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (339.5") between the two second-epoch detections
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Considering the candidate 289034_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289034_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (217.8") between the two second-epoch detections
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Considering the candidate 289036_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289036_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:39.29 +01:55:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.172 3114762887822871424 106.41268811776 +01.91781016527 13.9973 13.4948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289041_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289041_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:58.58 +02:45:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289042_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289042_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289044_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289044_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 289046_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289046_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:49.90 +02:29:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289047_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289047_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:15.45 +02:15:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289049_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289049_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (104.6") between the two second-epoch detections
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Considering the candidate 289051_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289051_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (430.3") between the two second-epoch detections
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Considering the candidate 289052_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289052_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289054_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289054_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:11.83 -02:02:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289056_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289056_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:07.05 +02:57:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.505 3115877826971729792 105.02857894626 +02.96449349911 13.9092 13.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:09.27 +02:42:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.515 3115801793168987008 105.53785657963 +02.70050759671 13.6587 13.1969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289058_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289058_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (41.4") between the two second-epoch detections
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Considering the candidate 289060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:54.79 +02:36:13.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 289066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:45.36 +02:52:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289067_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289067_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (71.9") between the two second-epoch detections
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Considering the candidate 289069_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289069_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:43.90 -04:10:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.290 3104610895101666816 096.93197827059 -04.17732097036 13.5523 12.7328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289074_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289074_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (155.5") between the two second-epoch detections
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Considering the candidate 289078_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289078_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 289080_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289080_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:46.53 -01:02:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289082_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289082_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289085_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289085_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:09.60 +03:04:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289087_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289087_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:43.74 -00:18:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289088_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289088_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:06.64 +00:28:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.888 3113392007278549888 103.27695675982 +00.46879719149 13.5732 13.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (274.4") between the two second-epoch detections
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Considering the candidate 289091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:37.32 +02:26:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.356 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289094_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289094_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:28.36 +02:18:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289095_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289095_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289097_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289097_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (145.9") between the two second-epoch detections
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Considering the candidate 289098_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289098_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:50.66 +00:09:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289102_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289102_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:25.84 -02:05:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.879 3108448289462234112 107.60725179185 -02.09678939304 13.6591 12.9545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289106_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289106_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:16.50 -02:07:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.144 3108444995228839296 107.81831127898 -02.12859756211 13.5607 13.0872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:31:48.12 -00:35:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.220 3119256626203802880 097.94986559533 -00.58771369680 13.3413 12.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289108_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289108_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 289114_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289114_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:37.66 -02:21:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289117_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289117_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (293.3") between the two second-epoch detections
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Considering the candidate 289118_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289118_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (50.9") between the two second-epoch detections
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Considering the candidate 289119_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289119_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 289121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (88.2") between the two second-epoch detections
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Considering the candidate 289122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:51.61 +02:28:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289123_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289123_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289127_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289127_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:49.54 +02:12:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.087 3126371020489836416 101.95615448199 +02.21651138326 13.3237 12.5073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289128_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289128_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:24.46 +02:31:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.846 3115933081729978112 106.85158664832 +02.52314265827 13.6716 13.1439 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#
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Considering the candidate 289130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:20.83 -00:46:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.924 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289131_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289131_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 289132_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289132_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:25.64 +02:12:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289135_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289135_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289143_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289143_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:34.69 +01:34:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.290 3114874007212799872 107.89391146696 +01.58006011879 13.6108 13.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289144_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289144_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289149_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289149_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (81.8") between the two second-epoch detections
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Considering the candidate 289152_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289152_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:53.67 +02:27:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289154_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289154_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (42.8") between the two second-epoch detections
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Considering the candidate 289156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:44.56 -01:00:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289157_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289157_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:42.96 +01:59:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.302 3114730692744947456 107.17833101923 +01.99528879820 13.2190 12.4774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289159_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289159_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:43.72 +02:46:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.504 3127766919219874688 104.18143344956 +02.78191443907 13.3299 12.8376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:41.55 -00:55:19.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 289162_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289162_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:58.07 +00:39:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.495 3114287490778891904 107.49132137484 +00.66128257443 13.4911 13.1180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289166_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289166_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:07.67 -00:37:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289167_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289167_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 289170_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289170_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (41.8") between the two second-epoch detections
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Considering the candidate 289171_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289171_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289173_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289173_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:37.25 -01:07:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.372 3110100481782530816 108.90476965786 -01.13221388038 13.4086 12.6729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:33.25 +00:32:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.921 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:42.56 +01:10:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289179_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289179_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:20.87 +00:20:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.795 3112961926432722688 104.58603893524 +00.34312302474 12.8940 11.9968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289180_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289180_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 289185_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289185_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289187_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289187_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289194_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289194_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:23.34 -00:49:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 3.526 3109432047432592384 107.84649073771 -00.82722994805 13.1589 12.4319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289195_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289195_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (137.4") between the two second-epoch detections
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Considering the candidate 289197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289199_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289199_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:19.53 -01:08:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289200_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289200_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289201_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289201_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:09.29 +00:52:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289203_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289203_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (32.8") between the two second-epoch detections
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Considering the candidate 289205_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289205_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:09.62 +00:41:52.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 289208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (131.5") between the two second-epoch detections
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Considering the candidate 289209_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289209_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289215_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289215_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:02.53 +01:07:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 3.842 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:36.77 -01:40:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.972 3109456094950953344 106.15260396703 -01.66850726094 12.9200 12.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289217_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289217_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:04.57 +00:48:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289220_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289220_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:54.74 +00:53:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.430 3113971690424905728 103.47724737496 +00.88351500760 12.1834 11.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289222_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289222_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:13.49 +01:52:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:46.06 +02:36:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.493 3127768293610081152 103.94127315085 +02.61504769689 12.8271 12.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289226_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289226_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:03.97 +02:40:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.438 3127770385254405888 104.01587799565 +02.67406252956 12.9076 12.4941 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 289227_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289227_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289233_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289233_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:13.90 -03:36:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.255 3102603805347108864 105.30706796189 -03.61185024820 12.7881 12.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289235_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289235_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:52.92 +00:49:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 2.743 3114539549519264128 105.96987120849 +00.82965293709 12.7423 12.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289236_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289236_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:18.52 -01:42:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.608 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289240_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289240_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:15.84 -02:22:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.167 3108833088474236544 106.06527567490 -02.38311151591 12.7621 12.4758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 289246_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289246_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (38.9") between the two second-epoch detections
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Considering the candidate 289250_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289250_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:01.02 -00:20:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289252_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289252_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:44.79 +02:19:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289253_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289253_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:33.41 -02:48:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 2.053 3108018247278107904 106.88869129625 -02.80810312876 12.3336 11.6435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:17.83 +01:47:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289258_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289258_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289260_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289260_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:50.98 -00:49:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289261_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289261_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:11.86 -01:33:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.522 3112276892032630400 103.29879130350 -01.56062176551 12.3437 11.9261 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#
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Considering the candidate 289262_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289262_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289265_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289265_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:26.75 -00:54:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 3.044 3112253325548814208 104.61066330762 -00.91453798124 11.7888 10.7799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289266_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289266_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (31.8") between the two second-epoch detections
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Considering the candidate 289267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:26.31 -02:18:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 289268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 289270_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289270_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:52.37 -01:57:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:37.57 +00:27:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 1.261 3114280412673080576 107.15620925738 +00.46477827338 10.8261 9.9927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289665_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289665_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:54.57 +01:33:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:12.42 -00:01:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289850_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289850_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:01.67 -00:05:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 1.663 3112865238129521920 104.75657781092 -00.08934525517 11.1791 10.2020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289868_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 289868_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:31.42 +01:47:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:37.34 +00:26:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 2.645 3113576308614129408 102.90501560737 +00.44942258340 11.7443 11.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290167_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290167_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (95.7") between the two second-epoch detections
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Considering the candidate 290171_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290171_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:39.83 +00:25:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.876 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 290182_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290182_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290222_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290222_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:37.80 +00:43:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 2.051 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 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#
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Considering the candidate 290255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:13.04 +02:40:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290321_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290321_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290364_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290364_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (118.4") between the two second-epoch detections
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Considering the candidate 290392_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290392_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:10.76 -03:14:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 2.520 3107892555054513664 106.04413364040 -03.24401870739 12.2870 11.8283 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 290427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:27.33 +02:30:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.933 3127192557534558720 101.11392637967 +02.51524587168 12.3802 11.9793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290439_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290439_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290455_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290455_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (374.1") between the two second-epoch detections
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Considering the candidate 290519_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290519_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290539_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290539_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:41.70 -00:33:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290547_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290547_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (141.5") between the two second-epoch detections
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Considering the candidate 290564_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290564_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:58.86 +02:49:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 3.608 3116003450473542784 106.49468568923 +02.82917133305 12.4156 11.5579 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 290565_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290565_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:11.49 -02:19:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:56.46 +00:49:07.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290622_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290622_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:43.29 +02:02:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290651_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290651_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (267.2") between the two second-epoch detections
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Considering the candidate 290658_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290658_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:35.72 +01:46:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 3.329 3114716777051331456 107.14809250164 +01.77852947417 12.4173 12.3215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.6") between the two second-epoch detections
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Considering the candidate 290667_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290667_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290724_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290724_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (159.7") between the two second-epoch detections
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Considering the candidate 290729_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290729_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:47.99 +00:39:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 1.969 3119814529571933824 099.69953942625 +00.66545390352 11.2963 9.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:53.87 +02:20:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290857_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290857_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:21.72 -03:19:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.271 3108623008734853504 105.59046160933 -03.32654619758 12.1808 10.8341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290864_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290864_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 290866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290866_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (184.4") between the two second-epoch detections
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Considering the candidate 290916_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290916_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:41.29 +00:46:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290922_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290922_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:15.96 +02:24:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.404 3126425545095312128 101.81640110765 +02.41641919175 12.5279 11.6391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:21:54.83 +02:22:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290938_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290938_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:28.57 -00:24:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290944_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290944_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (81.7") between the two second-epoch detections
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Considering the candidate 290958_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 290958_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:17.35 +02:00:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.487 3114765366020010752 106.57169428469 +02.00384672606 12.7577 12.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 290967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291018_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291018_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:37.60 +03:12:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.527 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291095_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291095_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:36.02 +00:49:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.535 3113827242086041984 104.89999945513 +00.83322365418 12.8202 11.8115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:10.49 +00:02:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.416 3112774390980328320 106.04409922559 +00.04009490383 12.8697 12.0978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291163_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291163_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291202_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291202_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291215_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291215_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:45.62 -02:10:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291249_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291249_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:26.53 +01:43:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291259_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291259_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291262_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291262_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:09.05 +00:16:36.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:11.87 -01:59:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:18.54 -05:24:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 4.312 3104187235226900352 096.82605277859 -05.40836792737 12.8062 12.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291301_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291301_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (351.7") between the two second-epoch detections
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Considering the candidate 291312_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291312_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:27.26 -00:49:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291349_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291349_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291400_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291400_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:59.93 +01:45:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291427_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:23.83 +00:54:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291437_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291437_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:00.32 -00:03:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.986 3107483197430678400 101.25075565208 -00.05928951009 13.0563 12.7107 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 291483_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291483_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291501_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291501_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291541_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291541_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:23.19 +00:25:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.532 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291544_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291544_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291606_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291606_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:52.36 +01:55:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291607_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291607_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:52.83 +00:17:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.999 3111447039926977152 109.46937545194 +00.28408061663 13.0457 12.6048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291625_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291625_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:13.69 +01:34:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.258 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291629_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291629_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:31.24 +00:46:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.839 3114351331172456192 106.87951415988 +00.76727923449 12.7081 11.6609 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 291673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291683_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291683_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:16.59 +02:11:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.285 3126229836324729216 103.31831126705 +02.19655818964 13.0960 12.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291700_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291700_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291707_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291707_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:08.14 -03:16:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.594 3108621599983160704 105.78322570098 -03.27201335860 13.1919 12.4770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291717_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291717_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 291767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 291771_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291771_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:38.60 +01:13:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291793_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291793_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291805_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291805_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (202.3") between the two second-epoch detections
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Considering the candidate 291812_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291812_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (314.9") between the two second-epoch detections
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Considering the candidate 291829_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291829_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (271.3") between the two second-epoch detections
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Considering the candidate 291842_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291842_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291844_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291844_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:24.34 +02:02:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (33.6") between the two second-epoch detections
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Considering the candidate 291862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
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Considering the candidate 291863_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291863_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (207.5") between the two second-epoch detections
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Considering the candidate 291896_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291896_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:54.77 -02:07:24.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)
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Considering the candidate 291901_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291901_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:55.24 +02:25:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.561 3126260828808488576 103.47941040606 +02.42500056399 13.2522 12.8317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:52.56 -00:27:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.923 3109706135063598592 106.71842488065 -00.45571211931 13.1534 12.3288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291941_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 291941_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 291960_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291960_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (147.2") between the two second-epoch detections
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Considering the candidate 291967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 291979_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 291979_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:54.37 +00:00:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.369 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (210.1") between the two second-epoch detections
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Considering the candidate 292012_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292012_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (223.9") between the two second-epoch detections
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Considering the candidate 292013_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292013_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:42.69 -00:02:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.292 3110635119311746688 110.67757703175 -00.03800331384 13.1481 12.6370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292027_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:23.08 +02:43:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292030_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292030_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 292033_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292033_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:02.40 +00:44:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.082 3111568192364065536 110.50993164837 +00.74401284736 13.4228 12.5402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292040_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292040_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:02.97 +02:23:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 3.836 3126248871620113792 104.01144429802 +02.38850732957 13.3451 12.7950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292063_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292063_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (212.2") between the two second-epoch detections
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Considering the candidate 292085_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292085_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 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 292099_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292099_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:38.80 +01:32:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:43.69 -00:29:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.549 3112692889681609088 106.18162536672 -00.49277504927 13.1660 12.3714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292111_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292111_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292119_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292119_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:53.44 -00:24:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 3.401 3112475323818314752 104.47188036842 -00.41113470113 13.3040 12.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292120_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292120_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:25.62 -01:40:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:17.61 -04:25:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292126_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292126_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (122.7") between the two second-epoch detections
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Considering the candidate 292129_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292129_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:03.44 -02:29:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 3.926 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.7") between the two second-epoch detections
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Considering the candidate 292174_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292174_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292177_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:09.25 +01:18:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292179_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292179_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (165.8") between the two second-epoch detections
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Considering the candidate 292189_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292189_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (283.4") between the two second-epoch detections
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Considering the candidate 292218_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292218_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:04.84 +02:28:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.797 3136010816885313280 110.01951799753 +02.47026567525 13.4213 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:40.01 +02:23:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292238_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292238_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:19.15 +02:16:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.492 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292254_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292254_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:28.83 -02:27:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292273_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292273_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292289_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292289_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:26.94 -01:43:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.465 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:22.58 -03:06:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 5.153 3108642426286693376 105.34338227084 -03.10135969197 12.9086 11.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292303_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292303_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292311_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292311_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:39.25 -02:16:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:26.09 -01:11:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.730 3110099691508601472 108.85787273649 -01.19101426949 13.5682 13.1534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292362_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292362_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:52.26 +00:59:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292373_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292373_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292401_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292401_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (95.8") between the two second-epoch detections
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Considering the candidate 292409_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292409_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:23.51 -01:37:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.246 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292472_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292472_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:22.22 -00:53:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.433 3112424230887731712 104.09176485857 -00.88726742447 13.5854 13.1578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292477_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292477_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:28.18 +01:29:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.317 3114638612946094336 106.36647147059 +01.49234473238 13.4661 12.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292494_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292494_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292526_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292526_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (97.5") between the two second-epoch detections
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Considering the candidate 292536_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292536_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:14.91 -02:18:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.395 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292551_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292551_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:55.21 -02:23:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:04.01 +02:09:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292592_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292592_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:39.07 -02:03:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292604_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292604_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292607_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292607_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292610_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292610_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:09.05 +02:19:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 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 292628_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292628_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:36.69 +02:42:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.885 3127764891995931648 104.15213331048 +02.71143748089 13.6251 13.1744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292639_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292665_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292665_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:14.17 -00:06:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.327 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292678_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292678_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:49.05 +01:06:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.187 3113111528733238784 105.45369517809 +01.10034936016 13.6098 13.2914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292687_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292687_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (142.8") between the two second-epoch detections
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Considering the candidate 292690_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292690_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:36.52 +02:34:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292703_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292703_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292708_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292708_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:23:57.70 -04:42:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (107.4") between the two second-epoch detections
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Considering the candidate 292730_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292730_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292761_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292761_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 292762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (30.9") between the two second-epoch detections
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Considering the candidate 292767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (85.1") between the two second-epoch detections
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Considering the candidate 292777_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292777_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (83.1") between the two second-epoch detections
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Considering the candidate 292778_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292778_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:11.75 +03:13:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.472 3127311480888772096 101.04831658328 +03.21883456912 13.4524 12.9837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292818_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292818_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:18.69 -00:51:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292819_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292819_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:11.70 -00:21:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292820_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292820_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:39.42 +02:22:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (209.7") between the two second-epoch detections
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Considering the candidate 292825_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292825_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:38.35 +02:11:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.947 3115718608241626880 104.40893150615 +02.18406946590 13.6140 13.1004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:36.16 +01:59:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:09.87 +01:21:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292845_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292845_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (137.6") between the two second-epoch detections
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Considering the candidate 292871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:31:37.07 +00:48:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.047 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (318.5") between the two second-epoch detections
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Considering the candidate 292898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:01.92 +00:03:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.882 3111202810908018432 107.75743753981 +00.06395802188 13.6799 13.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292904_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292904_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292943_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292943_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:32.38 +03:12:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.081 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292947_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292947_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292956_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292956_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292981_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 292981_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 292982_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 292982_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (133.2") between the two second-epoch detections
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Considering the candidate 293058_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293058_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:33.46 +01:51:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.581 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (157.1") between the two second-epoch detections
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Considering the candidate 293066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:04.93 +02:54:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293067_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293067_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:54.67 +00:45:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.437 3111384127245493376 107.97730601618 +00.76008378136 13.7155 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293069_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293069_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293080_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293080_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:08.04 +01:08:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:58.11 +01:31:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293100_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293100_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:33.06 -02:51:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293102_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293102_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:13.87 -00:07:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.246 3110295713814832000 109.55701383850 -00.12859499307 13.7200 13.1202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293105_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (81.5") between the two second-epoch detections
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Considering the candidate 293106_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293106_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (90.4") between the two second-epoch detections
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Considering the candidate 293122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:31.72 -04:05:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293127_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293127_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:59.83 -02:44:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293134_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293134_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:53.51 +03:13:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.589 3127291139925000832 100.97237071891 +03.21786171975 13.5859 12.7087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293139_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293139_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:38.96 +00:54:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.471 3113803014169734272 103.91154923036 +00.89978677975 13.7118 13.1253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293145_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293145_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (101.4") between the two second-epoch detections
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Considering the candidate 293158_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293158_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:10.04 +02:55:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293181_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293181_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293185_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293185_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:59.88 +00:10:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.511 3113319370792412800 103.74872486234 +00.18032112282 13.8383 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:04.52 -01:18:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.172 3109530659880536192 105.76838616188 -01.31131913292 13.7026 12.9785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293225_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293225_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:13.65 +00:52:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:00.20 -00:57:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.957 3109605181852110976 107.00017650752 -00.95349251268 13.5091 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293246_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293246_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293268_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (37.1") between the two second-epoch detections
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Considering the candidate 293269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293288_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293288_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (300.8") between the two second-epoch detections
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Considering the candidate 293295_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293295_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (123.8") between the two second-epoch detections
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Considering the candidate 293299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:20.64 -00:31:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293304_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293304_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293306_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293306_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:56.38 +01:32:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293314_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293314_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:59.67 -01:03:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.167 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 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 293329_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293329_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:22:43.72 -02:10:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293334_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293334_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:45.87 -02:11:00.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 293337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:53.19 +02:30:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.074 3126395102368111488 102.47096542506 +02.50276227856 13.8035 13.2960 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 293345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (309.3") between the two second-epoch detections
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Considering the candidate 293363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:40.07 +01:31:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:04.98 +02:42:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293383_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293383_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (155.4") between the two second-epoch detections
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Considering the candidate 293414_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293414_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:55.02 +00:08:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.254 3112896368052755200 105.22787396054 +00.14609736366 13.8402 13.0240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293424_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293424_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:08.32 +00:05:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293428_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293428_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:37.40 +01:48:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293432_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293432_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:28.14 +00:52:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293440_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293440_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293444_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293444_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:39.63 -00:16:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.891 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293461_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293461_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (125.9") between the two second-epoch detections
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Considering the candidate 293462_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293462_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:47.18 +01:57:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293464_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293464_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (211.5") between the two second-epoch detections
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Considering the candidate 293473_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293473_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293476_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293476_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293495_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293495_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 293507_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293507_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:25.11 +00:07:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.839 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293511_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293511_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293530_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293530_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:48.80 -02:49:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.923 3108008042435350144 106.45202773361 -02.82932879042 13.6288 12.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293534_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293534_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293554_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293554_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293563_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293563_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (72.1") between the two second-epoch detections
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Considering the candidate 293587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:34.85 -01:08:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293590_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:53.29 +01:49:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.937 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:24.68 +00:13:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293603_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:26.94 -00:55:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 0.719 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (53.3") between the two second-epoch detections
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Considering the candidate 293619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:33.29 +01:24:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.589 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (43.6") between the two second-epoch detections
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Considering the candidate 293630_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293630_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 293651_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293651_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:22.10 -00:32:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293662_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293662_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (109.2") between the two second-epoch detections
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Considering the candidate 293672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:26.05 -01:49:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293677_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293677_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293686_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293686_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (335.7") between the two second-epoch detections
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Considering the candidate 293696_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293696_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293716_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293716_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293718_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293718_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293721_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293721_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:33.88 -01:42:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293727_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293727_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293728_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293728_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293747_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293747_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:27:32.68 +01:54:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293789_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293789_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (235.8") between the two second-epoch detections
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Considering the candidate 293797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:21.13 -03:11:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293815_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293815_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293820_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293820_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:21.01 +01:42:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.371 3115443146220515200 105.08662575865 +01.70320261251 13.6660 12.7932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293821_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293821_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (126.7") between the two second-epoch detections
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Considering the candidate 293826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (409.0") between the two second-epoch detections
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Considering the candidate 293840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:27.15 -01:19:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293861_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 293868_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293868_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293869_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293869_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293887_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293887_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:25.30 -00:52:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293894_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:06.82 +01:33:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.918 3125769140951396608 101.77770849888 +01.56143873464 13.8938 13.1197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293900_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293900_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293908_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293908_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (87.2") between the two second-epoch detections
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Considering the candidate 293909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:03.47 -00:48:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.492 3109630955956555264 107.26411041079 -00.80830256355 13.9760 13.2107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (273.7") between the two second-epoch detections
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Considering the candidate 293925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (67.4") between the two second-epoch detections
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Considering the candidate 293931_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293931_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293933_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293933_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:26.44 -02:20:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.632 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293946_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293946_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293949_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293949_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:21.04 +01:51:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:36.03 +01:44:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293959_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293959_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293961_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293961_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:23.59 -00:09:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.614 3110294614303203840 109.59691543912 -00.15792757095 13.9002 13.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293963_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293963_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293966_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293966_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293970_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293970_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293975_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 293975_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 293980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:42.18 +03:11:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.716 3130161170208610688 098.92490276050 +03.18629758406 13.7622 13.1813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293993_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293993_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (253.3") between the two second-epoch detections
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Considering the candidate 293994_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293994_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:04.17 +01:58:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.408 3126360472050420992 101.76704300021 +01.97593177349 13.9878 13.4960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293996_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293996_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:10.52 -00:43:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.821 3119206774519517696 098.79348040669 -00.72377880410 14.0197 13.4537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293998_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 293998_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (127.7") between the two second-epoch detections
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Considering the candidate 294001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:39.57 -01:21:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.218 3109339619737041536 107.41478777276 -01.36419332163 13.8942 13.1712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294002_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294002_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:21.22 -01:43:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:38.70 -00:36:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.179 3109678956510644992 106.66014041170 -00.61650773442 13.7470 12.8165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294010_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294010_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:06.99 +01:28:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.159 3114813572733233536 108.52789238315 +01.47157397760 14.0252 13.5694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294023_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294023_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:34.40 -01:39:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294027_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294027_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294035_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294035_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 294036_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294036_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294044_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294044_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:46.11 -00:21:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.715 3111161544862117376 107.44144857121 -00.35527919213 13.8352 12.8859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294089_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 294090_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294090_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (45.2") between the two second-epoch detections
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Considering the candidate 294096_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294096_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294098_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294098_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:39.21 -01:16:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294136_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294136_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:11.77 +02:40:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294140_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294140_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:46.02 -01:37:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.735 3109460806533000320 106.19109724512 -01.61800116054 14.0008 13.0721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294143_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294143_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:54.83 +00:47:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294150_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294150_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294152_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294152_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (206.6") between the two second-epoch detections
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Considering the candidate 294153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (147.4") between the two second-epoch detections
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Considering the candidate 294156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294158_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294158_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.6") between the two second-epoch detections
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Considering the candidate 294160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 294183_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294183_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294190_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294190_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294197_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (79.6") between the two second-epoch detections
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Considering the candidate 294218_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294218_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294221_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294221_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294227_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294227_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
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Considering the candidate 294231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294231_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:41.54 -00:33:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.421 3112503842401083904 103.42233870049 -00.56409058978 14.0403 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294254_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294254_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (114.4") between the two second-epoch detections
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Considering the candidate 294255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294255_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:31.22 +01:34:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (310.7") between the two second-epoch detections
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Considering the candidate 294302_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294302_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:48.28 +02:38:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294313_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294313_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:44.88 -00:31:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.060 3110957482375863680 107.68635159393 -00.52085538438 13.9592 13.2293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294317_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294317_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294319_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294319_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294351_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294351_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:24.79 +02:20:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.486 3115118343612453632 107.60230636112 +02.33784729094 13.8710 13.1518 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 294360_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294360_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (63.7") between the two second-epoch detections
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Considering the candidate 294362_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294362_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294377_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294377_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294378_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294378_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:28.11 -01:46:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.452 3117534997152676096 097.11660672041 -01.77414040698 13.9213 13.4771 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 294379_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294379_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294386_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294386_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294401_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294401_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (118.0") between the two second-epoch detections
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Considering the candidate 294405_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294405_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294413_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294413_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294415_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294415_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294416_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294416_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294419_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294419_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:41.52 +02:07:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294420_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294420_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:02:01.17 -00:33:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.940 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294442_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294442_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:35.56 -00:48:25.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 294444_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294444_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294446_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294446_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294452_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294452_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:43.22 -01:01:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.440 3118951241146175232 099.42954310873 -01.02151054287 13.6241 12.5112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294470_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294470_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294471_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294471_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:40.33 -00:26:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.793 3112511367183611136 103.66730236160 -00.44919517720 13.9757 13.1957 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#
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Considering the candidate 294490_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294490_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 294494_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294494_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:23.85 +01:25:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.880 3125762818759967744 101.84877210392 +01.42791191353 14.1120 13.6271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294504_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294504_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
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Considering the candidate 294523_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294523_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:16.51 -02:05:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.420 3108855903340435200 105.81770007262 -02.09964696229 14.0457 13.5449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294524_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294527_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294527_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294557_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294557_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:15.65 -02:19:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.008 3108285566046423424 108.56429063089 -02.32885347419 13.8739 13.2100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294567_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294567_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:52.56 +01:12:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294571_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294571_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (117.7") between the two second-epoch detections
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Considering the candidate 294573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294581_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294581_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:53.09 -00:46:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294591_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294591_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294599_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294599_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (76.0") between the two second-epoch detections
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Considering the candidate 294601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294601_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:42:15.78 +01:14:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294605_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294605_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:07.16 +01:49:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.063 3115421087268758272 105.77929704766 +01.82442252696 14.0333 13.6803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:38.17 +02:58:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.542 3127807566790246656 104.15815265319 +02.97090946993 14.1540 13.2807 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 294645_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294645_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:28:13.98 +01:53:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 294648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:05.27 +02:32:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294660_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294660_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294672_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (384.9") between the two second-epoch detections
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Considering the candidate 294673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294673_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:35:50.23 -02:34:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294694_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294694_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (95.5") between the two second-epoch detections
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Considering the candidate 294696_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294696_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294698_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294698_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294699_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294699_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (102.8") between the two second-epoch detections
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Considering the candidate 294706_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294706_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:08.81 -03:48:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.375 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294708_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294708_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294732_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294732_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (158.9") between the two second-epoch detections
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Considering the candidate 294735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294745_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:02.99 +01:17:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.710 3114067687234902528 103.26150189626 +01.29007914832 14.2536 13.7674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294752_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294752_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294754_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294754_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (59.9") between the two second-epoch detections
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Considering the candidate 294755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:13.96 +02:27:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294762_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (98.3") between the two second-epoch detections
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Considering the candidate 294767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (255.5") between the two second-epoch detections
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Considering the candidate 294776_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294776_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294777_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294777_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (218.2") between the two second-epoch detections
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Considering the candidate 294784_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294784_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (167.3") between the two second-epoch detections
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Considering the candidate 294788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294788_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (86.0") between the two second-epoch detections
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Considering the candidate 294791_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294791_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (42.9") between the two second-epoch detections
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Considering the candidate 294794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294795_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294795_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:18.73 +00:22:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.446 3111309188656981760 108.07730307100 +00.38111351250 14.2369 13.6868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:31.45 +02:25:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.270 3126956441710853888 099.63043614299 +02.42681295214 14.2095 13.6254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:53.17 +02:16:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.825 3126232241506271744 103.47069199047 +02.27525024279 13.8274 12.8883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294817_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294817_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:17.39 -00:43:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.038 3110935006809228800 108.07150437030 -00.72003445389 14.2336 14.0671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294823_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:43.29 +01:18:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.871 3114478256045530880 107.18018799747 +01.30027429888 14.1885 13.8027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294831_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294831_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:34.17 +00:00:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294838_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294838_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294843_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294843_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294844_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294844_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:44.97 -01:27:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.463 3109290210433083904 107.18641627578 -01.46642509877 14.0670 13.2431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294876_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294876_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294880_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294880_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:05.85 +03:07:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.930 3130145334667135232 099.27333575975 +03.13107873566 14.1676 13.5769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294885_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294885_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:13.39 +00:50:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.651 3125567827244921728 101.55524044974 +00.83678768778 13.7948 12.7251 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#
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Considering the candidate 294886_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294886_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:19.19 +03:02:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.114 3127835398178483712 103.82909987491 +03.03343876125 14.1871 13.7059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294907_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294907_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 294912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294915_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294915_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:17.63 +00:47:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.750 3111710128145058304 109.07248660846 +00.79791269027 14.2761 14.0748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294916_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294916_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:58.53 +01:29:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.568 3125767182446332672 101.74323261975 +01.48735629924 14.0034 13.4904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294935_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:49.28 +01:22:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294968_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294968_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:47.27 -01:24:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.378 3109165140984226176 105.44692959018 -01.41554928022 14.1477 13.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294971_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294971_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:34.46 -02:33:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294980_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:29.09 -01:37:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294988_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 294988_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 294990_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 294990_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:59.01 +00:22:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.581 3112953473937328256 104.99505493550 +00.36980486509 14.2939 13.9155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295008_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295008_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:44.83 +00:19:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.787 3113526937970401024 101.93613473648 +00.32181602988 14.2790 13.5395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295046_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295046_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:15.33 +02:57:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 0.529 3127277567827167744 100.81373491645 +02.96379530653 14.2431 13.6127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295055_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295055_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (95.0") between the two second-epoch detections
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Considering the candidate 295056_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295056_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (197.3") between the two second-epoch detections
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Considering the candidate 295086_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295086_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (37.5") between the two second-epoch detections
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Considering the candidate 295087_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295087_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (276.2") between the two second-epoch detections
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Considering the candidate 295104_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295104_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 295139_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295139_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:40:57.05 -04:34:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.587 3103787734552535808 100.23751504165 -04.58187315124 14.1352 13.3718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295140_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295140_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295146_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295146_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (211.6") between the two second-epoch detections
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Considering the candidate 295147_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295147_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295153_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (114.8") between the two second-epoch detections
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Considering the candidate 295165_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295165_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295202_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295202_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:56.87 -01:56:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295207_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295207_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:53.97 +01:06:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.444 3125683344685580672 102.47375912103 +01.10491595488 14.1722 13.6700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295213_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295213_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 295216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295217_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295217_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (279.4") between the two second-epoch detections
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Considering the candidate 295224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295224_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:55.91 +02:12:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.387 3115534749282919808 106.23258178573 +02.21434297826 14.3534 13.6137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295232_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295232_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (42.2") between the two second-epoch detections
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Considering the candidate 295238_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295238_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295249_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295249_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:56.12 +03:05:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.778 3127144733077191168 099.48283186955 +03.08662636258 14.3388 13.7231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295253_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295253_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295258_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295258_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.8") between the two second-epoch detections
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Considering the candidate 295267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295267_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:02.74 -00:42:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.131 3109627588701789184 106.76082783589 -00.70808447428 14.2295 13.7367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295269_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 295275_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295275_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:07.11 +02:25:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:59.07 -00:56:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.249 3110001250859064192 110.24535678933 -00.93603487251 14.2713 13.9796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295314_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295314_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:26.86 +02:20:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.045 3115560244208643584 106.36121092667 +02.33390289189 14.3152 13.4731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295316_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295316_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (282.1") between the two second-epoch detections
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Considering the candidate 295324_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295324_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:20.72 +01:13:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.316 3125864244409403520 100.33543376487 +01.22093941297 14.2202 13.4847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295330_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295330_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (137.6") between the two second-epoch detections
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Considering the candidate 295332_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295332_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:27.05 -02:25:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295339_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295339_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:56.57 +02:14:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295353_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295353_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:58.75 +00:23:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.652 3113693342185540992 104.24362456898 +00.39639448205 14.3425 13.7304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295389_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295389_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:18.01 +02:44:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295393_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295393_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (154.0") between the two second-epoch detections
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Considering the candidate 295411_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295411_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295413_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295413_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:18.91 +00:11:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.295 3111125531558570240 108.82810029911 +00.18605547641 14.2785 13.9157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295422_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295422_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295424_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295424_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:20.45 -00:32:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.956 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295430_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295430_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 295459_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295459_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295461_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295461_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295462_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295462_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (213.9") between the two second-epoch detections
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Considering the candidate 295465_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295465_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (122.7") between the two second-epoch detections
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Considering the candidate 295474_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295474_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295489_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295489_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:11.66 +02:43:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.161 3115215856549696896 107.54800627027 +02.72608749165 14.4383 13.9485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295497_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:01:15.85 -02:12:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.914 3109049589185408896 105.31471997974 -02.21526180554 13.8444 12.8572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295503_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295503_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:34.77 +00:32:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.483 3113580985840503296 103.14371971951 +00.54139619495 14.0748 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295506_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295506_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (88.0") between the two second-epoch detections
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Considering the candidate 295520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295535_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295535_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:14.43 -02:35:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.077 3108028589559012352 107.05873851832 -02.59207168230 14.4695 14.1766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295549_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295549_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:17.86 +01:26:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295555_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295555_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295562_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295562_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:46:57.63 -02:12:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.102 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295586_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:28.56 -00:06:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.640 3113342116939096320 102.86798069500 -00.10932871864 14.4085 13.8585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295588_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295592_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295592_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295600_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295600_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:00.91 +02:07:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.772 3126357757630860032 102.00302124251 +02.12552770298 14.1601 13.2341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295602_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295602_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295609_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295609_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:42.51 +01:09:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.666 3113865656273175808 105.17619282814 +01.15358932891 14.3494 13.4480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295617_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295617_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295618_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295618_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:43.56 +03:08:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295621_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295621_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295625_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295625_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 295632_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295632_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 295636_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295636_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (137.8") between the two second-epoch detections
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Considering the candidate 295642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295648_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295649_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295649_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295659_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295676_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295676_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (275.9") between the two second-epoch detections
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Considering the candidate 295682_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295682_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:34.40 +02:05:20.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 295684_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295684_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (104.8") between the two second-epoch detections
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Considering the candidate 295692_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295692_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295693_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295693_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (82.0") between the two second-epoch detections
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Considering the candidate 295701_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295701_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295709_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295709_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295711_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295711_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:47.14 +02:00:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.698 3120966405442532992 098.44606364458 +02.00309091251 14.4047 13.5826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295715_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295715_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295716_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295716_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:56.22 +00:47:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.513 3111387593283428096 107.98388188751 +00.79529565715 14.3369 13.8343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295722_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295722_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 295735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295735_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:36.93 +02:07:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.696 3115107863892490112 107.40311506479 +02.11780922257 14.1897 13.4324 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 295743_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295743_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (91.2") between the two second-epoch detections
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Considering the candidate 295755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295755_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:58:52.06 +02:39:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.595 3115772037634406400 104.71584183846 +02.65178183789 14.3006 13.6104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295760_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:02.17 -02:05:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.748 3108307556279925888 109.00858548489 -02.09969414457 14.3381 13.6119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295761_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295761_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:05.66 +00:51:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.278 3113605484332811648 103.02252679260 +00.85637243039 14.3468 13.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295769_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295769_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:48:54.41 +02:49:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295778_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295778_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (183.4") between the two second-epoch detections
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Considering the candidate 295798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 295809_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295809_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295811_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295811_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295822_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295822_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:38.94 +00:36:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.680 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295826_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:09.31 -00:13:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.285 3119287348105304320 098.53848301471 -00.22784823901 14.4685 13.8394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295834_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295834_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:40.27 +01:41:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.834 3114705580076209792 107.41698425144 +01.69019420898 14.5129 13.7544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295837_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295837_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 295838_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295838_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295840_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (155.1") between the two second-epoch detections
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Considering the candidate 295852_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295852_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:34:54.35 +01:23:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.348 3120676855925773696 098.72578573357 +01.39802428046 13.2177 11.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295853_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295853_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295862_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:59:17.89 -01:38:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.331 3112131588996763520 104.82504758752 -01.64439181385 14.3927 13.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (197.0") between the two second-epoch detections
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Considering the candidate 295871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295871_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (88.9") between the two second-epoch detections
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Considering the candidate 295903_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295903_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295909_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:42.17 +01:42:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (150.0") between the two second-epoch detections
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Considering the candidate 295922_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295922_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:47.86 +02:10:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.578 3135939864025973504 110.44901119712 +02.16671520657 14.5047 14.0354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295933_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295933_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:47:28.86 -01:01:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.068 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295939_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295939_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:32.03 +02:21:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.996 3126292336688152960 102.88280762511 +02.35264716426 14.2305 13.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295948_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295948_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 295955_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295955_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:00:26.60 +02:39:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.910 3115716821534660224 105.10986025612 +02.66309898479 14.3900 13.8357 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#
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Considering the candidate 295967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295967_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:39.84 +01:55:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.072 3111910999473783296 110.16485137981 +01.91823889181 14.3461 13.8057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295971_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295971_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (336.4") between the two second-epoch detections
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Considering the candidate 295990_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 295990_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:44.40 +02:44:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295992_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 295992_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296025_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296025_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:26.09 -02:19:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.523 3108810204889213440 106.35814706162 -02.32470763478 14.4457 13.9271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:18.32 -02:07:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.840 3106051805090685696 103.57553630608 -02.12473732458 14.3576 13.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296031_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296031_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296032_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296032_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296040_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296040_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (118.3") between the two second-epoch detections
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Considering the candidate 296042_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296042_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:35.50 +01:41:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.943 3114856041369812992 108.39690518346 +01.69802301952 14.2746 13.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296051_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296051_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 296078_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296078_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296079_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296079_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 296090_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296090_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (55.9") between the two second-epoch detections
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Considering the candidate 296091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296091_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296115_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:34.46 -01:09:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.695 3112325648499548032 103.64279549227 -01.15626921023 14.5400 13.9947 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 296123_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296123_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:28.97 +01:58:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.655 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296130_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296132_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296132_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296133_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296133_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:34.78 +02:05:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.119 3111975458339069952 109.39402841288 +02.08688917552 14.4678 13.7565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296135_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296135_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296157_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296157_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296160_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (47.5") between the two second-epoch detections
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Considering the candidate 296166_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296166_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:26.91 +01:30:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.366 3114673694239105408 107.11091176573 +01.50243433392 14.3921 13.6375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296182_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296182_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:20.89 +01:12:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.105 3111796993861960320 108.58609529900 +01.20097492060 14.3150 13.5711 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 296184_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296184_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:37:19.22 +00:16:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.427 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296188_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296188_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (64.1") between the two second-epoch detections
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Considering the candidate 296191_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296191_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:24.07 +00:46:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.546 3113040846452578560 105.84923126042 +00.78170329925 14.6307 14.0708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296214_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296214_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:51:32.67 +03:04:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.900 3126543437655686784 102.88541336288 +03.06712667176 14.4822 13.9993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296223_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:49:52.19 +00:49:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.924 3113659944517871104 102.46656884662 +00.83187008901 14.3851 13.8439 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 296228_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296228_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296239_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296239_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296240_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296240_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296257_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296257_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296259_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296259_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296265_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296265_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296273_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296273_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296278_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296278_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (61.8") between the two second-epoch detections
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Considering the candidate 296281_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296281_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:26:54.39 +00:14:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.613 3120219252930306048 096.72630679240 +00.23865925387 14.0808 13.1630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296284_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296284_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (286.2") between the two second-epoch detections
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Considering the candidate 296287_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296287_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:18.57 +00:08:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.362 3111068876647108224 109.32611179926 +00.14271098473 14.4796 14.1904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296292_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296292_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (147.1") between the two second-epoch detections
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Considering the candidate 296294_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296294_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:59.84 -01:25:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.650 3110030181758541312 109.24834244371 -01.42013320537 14.4440 13.9575 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 296299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296299_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296302_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296302_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:24.11 -01:31:48.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 296305_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296305_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296324_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296324_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296328_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296328_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 296337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296337_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (100.7") between the two second-epoch detections
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Considering the candidate 296341_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296341_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:29.65 +02:37:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.276 3126318381370054400 103.62266296559 +02.62664940288 14.3375 13.3693 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 296347_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296347_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296354_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296354_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (65.8") between the two second-epoch detections
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Considering the candidate 296359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 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 296361_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296361_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (198.0") between the two second-epoch detections
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Considering the candidate 296363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296363_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 296365_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296365_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:34.47 -02:44:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.207 3108030685503515904 106.64289710645 -02.73679236802 14.4500 14.2824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296369_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296369_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296376_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:33.65 +02:43:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.703 3115954590926082944 106.88907883203 +02.71761943078 14.4306 13.7145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296378_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296378_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:12.36 -01:00:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.229 3109990942939026304 110.55133284752 -01.01238137083 14.6172 14.1962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296381_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296381_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
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Considering the candidate 296385_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296385_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:38:49.97 +02:05:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296390_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296390_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:00.92 -02:29:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.769 3108405378450160640 107.25314373552 -02.49393719618 14.0537 13.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296392_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296392_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296411_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296411_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:38.39 +00:20:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.284 3110698375589262336 110.65906151209 +00.33269006405 14.5957 14.0697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296414_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296414_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (146.7") between the two second-epoch detections
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Considering the candidate 296419_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296419_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:17.49 +00:27:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.423 3114270895025725184 106.82187194807 +00.45551255670 14.5636 14.0473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296423_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296423_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296425_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296425_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:57:02.34 +02:04:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296433_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296433_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:40.11 +02:28:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.306 3115565943624832512 106.41606503327 +02.47127709305 14.6161 14.2360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296435_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296435_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:43.35 -02:05:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.004 3106941413077711360 101.17994342396 -02.10121165387 14.0609 13.1706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296437_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296437_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:48.77 +01:08:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.596 3114460041087267584 107.45277958901 +01.14037546146 14.6788 14.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296439_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296439_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:31.53 +00:02:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.344 3111052177814297856 109.38074301715 +00.03593027805 14.4272 13.9108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296440_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296440_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (49.5") between the two second-epoch detections
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Considering the candidate 296443_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296443_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296445_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296445_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296446_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296446_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296450_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296450_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296451_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296451_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:10.28 +00:45:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.254 3113646750379142400 102.54192353963 +00.75016248721 14.5407 13.9477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296454_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296454_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296463_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (58.1") between the two second-epoch detections
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Considering the candidate 296472_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296472_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 296476_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296476_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:42.02 -00:14:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.671 3112530196319963392 104.17392800786 -00.24495175114 14.5389 13.9379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296477_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296477_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296479_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:14.55 -02:26:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.119 3108411803721141632 107.30972146437 -02.44456392592 14.4345 14.1385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296485_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296485_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:23.00 -01:48:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.089 3109790453866020736 109.84522423461 -01.81034772311 14.5757 13.9185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296490_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296490_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296493_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296493_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:16.91 +02:23:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296495_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296495_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (109.3") between the two second-epoch detections
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Considering the candidate 296496_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296496_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296500_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296500_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:22:33.21 -00:03:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.159 3110633538763804032 110.63754631751 -00.06241601560 14.6231 14.1269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296502_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296502_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296506_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296506_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (144.6") between the two second-epoch detections
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Considering the candidate 296514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296514_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:36.74 +00:53:46.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 296516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296516_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296517_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 296520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296520_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:53:04.81 -01:03:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.055 3112379288350193664 103.26910536434 -01.05934868750 14.2216 13.2133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296527_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296527_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:24:04.08 +00:07:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.000 3120250245414690688 096.01594473948 +00.13095788641 14.3800 13.4578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296532_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296533_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:16.61 -00:44:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.046 3110233247810795392 109.31903231866 -00.74722396746 14.5977 14.1484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296535_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296535_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (63.5") between the two second-epoch detections
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Considering the candidate 296539_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296539_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:30:03.90 -01:08:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.536 3119111082648138368 097.51558708996 -01.14316942859 14.5038 13.9128 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 296545_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296545_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296565_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296565_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (325.6") between the two second-epoch detections
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Considering the candidate 296566_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296566_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296569_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (221.3") between the two second-epoch detections
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Considering the candidate 296570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296570_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:26.12 +00:37:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.907 3111521291321446784 109.35805151725 +00.62458059794 14.5371 14.0204 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 296573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296573_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296575_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:14.20 +01:06:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296579_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296579_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296587_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:01.74 -02:19:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.372 3108836593167546880 106.00616135184 -02.33220666900 14.2876 13.4376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296594_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296594_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296599_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296599_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (286.7") between the two second-epoch detections
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Considering the candidate 296614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296614_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296619_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296623_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296626_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296626_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296631_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296631_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:02.87 -02:22:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.386 3108375141881723008 108.26112843601 -02.38233723579 14.4210 14.2296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296633_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296633_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:17.04 -01:11:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.086 3109418887653270016 107.57010348959 -01.18670329760 14.6177 14.1411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296634_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:59.07 -01:35:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.411 3109319789866103424 107.49527235980 -01.59777488220 14.4699 13.9552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296635_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296635_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:29.82 +01:25:12.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)
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Considering the candidate 296636_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296636_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (106.4") between the two second-epoch detections
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Considering the candidate 296642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296642_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:03.71 +00:49:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.436 3113967807774483072 103.51442571846 +00.82388324853 14.4966 13.9552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296644_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 296654_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296654_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:04.22 +00:51:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.108 3111543449054388224 109.76660457112 +00.85377407971 14.6094 13.7679 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 296655_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296655_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296656_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296656_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296661_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296664_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296664_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:32.57 -00:41:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.564 3110941230220145664 108.13457979217 -00.69024448427 14.4578 13.7600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296668_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296668_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296671_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296671_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (92.5") between the two second-epoch detections
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Considering the candidate 296675_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296675_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (319.1") between the two second-epoch detections
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Considering the candidate 296693_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296693_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296699_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296699_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296700_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296700_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:22.38 +00:16:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.880 3113684683531570816 104.09213995330 +00.27316633457 14.4415 13.6444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296702_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296702_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:32.17 +01:43:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.982 3114132116042404992 104.13313489612 +01.71856052911 14.4968 13.8059 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#
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Considering the candidate 296707_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296707_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296710_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296718_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296718_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296719_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296719_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:39:59.43 +00:54:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296726_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296736_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296736_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296740_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296740_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296741_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296741_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296744_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296744_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:25.03 -00:17:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.791 3109712659115220864 107.10346404505 -00.29265099079 14.4327 14.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296749_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296749_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296751_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296751_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:55.45 -03:00:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.515 3107988487450594048 106.72981799531 -03.00561584569 14.7390 14.4495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296753_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296753_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:59.47 -02:29:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.141 3108381429714126592 107.74675809943 -02.48586767073 14.2019 13.4283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296757_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 296758_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296758_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:23.75 +01:08:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.506 3114413797176923776 107.59836638225 +01.13542481352 14.6575 14.3803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296759_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296759_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:52.11 -00:30:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296763_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296763_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:23.21 +00:09:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.486 3111113540009777664 108.84579160620 +00.15396145097 14.5883 14.0016 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 296767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296767_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296768_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296768_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:56.87 -01:44:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.224 3109827665462982912 109.23614501145 -01.74778549119 14.5731 14.1670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296771_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296771_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:25.93 +02:53:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.427 3127783583692946688 104.10705211273 +02.89351819734 14.5242 13.8965 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 296775_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296775_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:43.04 -01:37:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.798 3109275470105089536 106.42843589909 -01.62277730617 14.5701 14.2314 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#
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Considering the candidate 296780_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296780_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:45:06.22 +02:35:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.302 3127193833145620992 101.27555581414 +02.58608371871 14.6006 14.1219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296781_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296781_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:43.33 -00:06:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 3.824 3110659480365896064 110.17967027544 -00.11727397717 14.4936 13.9989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296782_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (357.7") between the two second-epoch detections
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Considering the candidate 296794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296794_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (55.6") between the two second-epoch detections
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Considering the candidate 296797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296797_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296798_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296799_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:17.49 +00:40:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.150 3111335125961382912 108.82182231826 +00.67266901497 14.6425 14.1192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296806_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296806_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296807_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296807_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:11.69 -00:40:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.536 3112595028846552064 106.04822651650 -00.66768070523 14.2934 13.4200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296814_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296814_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (41.5") between the two second-epoch detections
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Considering the candidate 296816_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296816_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:25.10 -02:34:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.193 3060191965371506048 109.60372468714 -02.56707972742 14.3748 13.5629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296817_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296817_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:45.53 -00:30:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.100 3109701152901485184 106.93905211362 -00.51141863229 14.7704 14.3372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296818_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296818_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:08.68 -00:01:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.785 3111232837019910656 107.03525090547 -00.03362767301 14.2683 13.7055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296830_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296830_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:33.59 +02:09:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.676 3126238460618897792 103.63897544738 +02.16303910243 14.5450 13.9446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296832_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (262.3") between the two second-epoch detections
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Considering the candidate 296833_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296833_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:17.07 -00:40:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.244 3109452388397346432 107.57064704324 -00.67812218674 14.7762 14.3621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296845_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296845_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296863_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296863_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:10:30.37 +00:54:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.977 3114394620144340224 107.62649990680 +00.91524048004 14.5090 14.2477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296865_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296865_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (122.0") between the two second-epoch detections
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Considering the candidate 296867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296867_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296869_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296869_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296870_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:13.56 +01:07:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296879_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296882_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296882_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296884_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296884_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:06:39.01 -01:53:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.509 3109252895757025920 106.66172268544 -01.88689027584 14.4879 13.9728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296888_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296888_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (46.5") between the two second-epoch detections
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Considering the candidate 296892_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296892_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:33.75 -01:33:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.928 3108538724296809472 108.64006745489 -01.55987007368 14.3642 13.5349 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 296893_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296893_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:36.31 +02:13:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.574 3114960357534918656 109.15046816890 +02.21911136278 14.5890 13.8884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296896_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296896_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:34.42 +00:12:45.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 296898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296898_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296901_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296901_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296902_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296902_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (119.8") between the two second-epoch detections
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Considering the candidate 296913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296913_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:29.11 +02:57:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.474 3127269493289321088 101.12157744479 +02.96576563252 13.8513 12.4359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296925_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:47.59 +02:02:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.785 3115102160176677376 107.44748614861 +02.03332384108 14.3920 13.8433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296930_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296930_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:52.78 +01:42:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.088 3114855697772402048 108.46912999652 +01.70740690773 14.5770 14.0373 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 296937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296937_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (179.3") between the two second-epoch detections
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Considering the candidate 296942_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296942_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:29.23 -00:27:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.126 3110969714442949248 108.37096740466 -00.45916189891 14.6390 13.9015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296949_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296949_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296952_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 296976_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296976_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:43:25.89 -02:45:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.120 3105759025758656640 100.85689686409 -02.75826249440 14.5773 14.1335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296978_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296978_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:18:29.70 +01:56:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.703 3111957385120256768 109.62303490316 +01.93393434793 14.7591 14.3576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296984_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 296984_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:44.71 +01:32:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.135 3114817863403426688 108.43547051635 +01.53551446979 14.5506 14.0352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296988_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 296988_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297001_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:26.00 +00:20:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.373 3110709542504465024 110.10728596609 +00.34594021175 14.4427 14.0015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297003_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297003_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:49.56 +02:01:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.828 3114950771168057344 108.95602724621 +02.02709205202 14.5616 13.8623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:31.70 -01:18:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.555 3110094090871416704 108.63105422730 -01.30851405220 14.7359 14.3022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297009_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297009_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:11:28.44 -02:06:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.929 3108444960869046656 107.86744153867 -02.11742510029 14.5734 14.1073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297021_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297021_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297028_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297029_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297029_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:21.11 +00:12:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.482 3111434326824067840 109.83730776348 +00.20836744744 14.7351 14.0107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297048_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297048_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:55:32.30 +01:33:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.615 3114123113791161984 103.88347927431 +01.56090348449 14.6417 14.1184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297050_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297050_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:21:24.21 -00:37:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.248 3110204488710611968 110.35022641615 -00.62546066998 14.4817 14.1062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297057_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297059_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297059_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:33.38 -00:14:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.865 3110982079649630208 108.38842305050 -00.24951329506 14.5535 14.1492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297060_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:29.67 +01:16:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.677 3114663004060893696 106.87273965152 +01.27246564929 14.3397 13.5666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297061_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297061_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:56:28.82 +02:36:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.065 3127757298493774976 104.11925300872 +02.61567810021 14.4555 13.6028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297064_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297064_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:44.63 +02:19:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.733 3114996534040216448 109.18495021955 +02.32139210549 14.4606 13.7466 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 297066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297066_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:15:30.57 -00:11:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.694 3111033279958582400 108.87667733520 -00.18803026937 14.4053 13.8506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297073_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297073_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:48.32 -02:30:00.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 297074_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297074_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:07:32.41 -01:29:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 5.348 3109292787412965504 106.88366036045 -01.48538103804 14.4719 13.6970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297075_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:41:32.31 +02:29:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.522 3126852228625127808 100.38410220975 +02.48272834843 14.6491 14.0474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297082_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297082_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (158.5") between the two second-epoch detections
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Considering the candidate 297083_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297083_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297099_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297099_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:12.65 +00:31:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.878 3111338634952385664 108.55152593704 +00.53147685523 14.6607 14.0814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297101_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297101_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297107_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 297108_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297108_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:16:17.26 -01:12:35.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 297111_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297111_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:07.42 -02:41:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.871 3108175065129915520 108.02956215298 -02.69563296753 14.6384 14.1585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297121_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:05:22.78 -01:37:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.153 3109462966898813184 106.34401149466 -01.61788220358 14.4979 13.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297125_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297125_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297129_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297129_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:52:55.62 +02:25:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.214 3126288144800632704 103.23117106246 +02.43214891333 14.2134 13.1860 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 297137_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297137_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 297138_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297138_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:04.42 -01:16:36.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 297142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297142_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:14:33.29 -01:27:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.624 3110087596880945536 108.63750355090 -01.45183557752 14.4490 14.0041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297147_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297147_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (134.9") between the two second-epoch detections
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Considering the candidate 297149_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297149_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:20:31.63 -00:31:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.310 3110209780109641216 110.13082174114 -00.52475736375 14.7022 14.0037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297162_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297162_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (96.2") between the two second-epoch detections
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Considering the candidate 297163_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297163_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297165_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297165_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (145.2") between the two second-epoch detections
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Considering the candidate 297172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297172_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:44:38.04 -00:15:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.277 3107470415608172672 101.15808190840 -00.25544744629 14.6389 13.7194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297175_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (122.8") between the two second-epoch detections
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Considering the candidate 297178_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297178_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297180_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297180_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:04:31.86 +01:55:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.980 3115510766186243968 106.13179332087 +01.91847299634 14.7238 14.1412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297183_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297183_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (53.6") between the two second-epoch detections
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Considering the candidate 297189_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297189_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297192_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297192_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 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 297208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297208_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:13:57.34 +01:10:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.553 3111797200020454144 108.48779788381 +01.17513238934 14.5898 14.3020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297211_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297211_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:17:20.03 +00:15:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.464 3111072312620878336 109.33277778656 +00.25885233590 14.6569 14.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297216_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:54:12.43 -03:32:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 5.096 3102758252370218624 103.55070839453 -03.54469153497 14.3280 13.3809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297230_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297235_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297235_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297236_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297236_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (76.1") between the two second-epoch detections
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Considering the candidate 297237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297237_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:08:48.02 +00:06:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.536 3111241603051546624 107.19919363648 +00.09963927044 14.6134 14.0641 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 297239_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297239_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (227.1") between the two second-epoch detections
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Considering the candidate 297241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297241_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (128.0") between the two second-epoch detections
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Considering the candidate 297244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297244_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (57.3") between the two second-epoch detections
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Considering the candidate 297251_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297251_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297264_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 297264_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 297285_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297285_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:03:48.88 -01:24:41.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
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Considering the candidate 297290_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297290_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:12:28.05 -02:41:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 297326_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297326_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 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 297345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297345_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (90.6") between the two second-epoch detections
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Considering the candidate 297399_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 297399_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (116.4") between the two second-epoch detections
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Considering the candidate 63434_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 63434_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (131.3") between the two second-epoch detections
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Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:19:38.85 -02:00:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 91187_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 91187_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:29:54.02 -03:35:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 154583_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 46178_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 46178_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:50:00.85 +01:46:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 3.726 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (206.8") between the two second-epoch detections
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Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 121122_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 07:09:13.75 -02:21:30.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 67537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 67537_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 270041_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 270041_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (128.3") between the two second-epoch detections
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Considering the candidate 78004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 78004_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
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Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (305.1") between the two second-epoch detections
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Considering the candidate 184359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 184359_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
**** FOUND 06:33:07.58 -00:02:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.174 3120055253898479360 098.28079145561 -00.03474886862 14.0993 13.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
Preparing report for the candidate 131156_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 31804_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (83.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47889_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030
The candidate 47889_fd_Mon-02-Q1b1x1_2026-04-15_21-43-17_20.00sec_-4.90C_LIGHTs_0030 did not pass the final checks
Rejecting candidate due to large distance (68.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 29s
make_report_in_HTML.sh TOTAL: 860s
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 ####
07:09:13.73 -02:21:30.2
07:05:28.89 -02:00:10.0
06:41:59.31 -01:11:07.3
07:08:45.38 +00:41:47.6
07:17:31.31 +01:05:38.1
07:06:47.77 -02:29:52.1
06:46:26.73 +00:59:01.5
07:02:38.04 -00:50:21.9
07:06:28.80 -02:56:50.2
06:46:22.32 +01:50:05.6
06:46:25.15 +01:49:06.0
06:44:06.85 -00:12:06.2
06:43:22.55 +02:17:18.7
06:50:17.33 +02:23:27.3
07:05:25.69 -00:15:24.7
07:02:13.97 -01:26:47.7
06:47:57.05 +02:21:35.4
06:37:46.58 +01:47:14.8
07:02:18.17 +01:30:39.3
07:09:29.63 -02:28:31.9
06:43:22.75 +01:54:53.9
07:18:59.78 -00:08:13.5
07:03:41.13 -02:10:56.7
07:07:26.39 +01:04:08.9
07:01:30.56 +00:16:28.3
07:02:25.57 -01:07:14.1
07:15:02.37 -01:57:47.6
07:06:11.37 +00:35:33.6
07:19:50.64 +00:15:40.1
06:46:19.51 -01:57:15.3
06:37:32.00 +01:46:25.8
07:01:58.24 -02:16:30.3
07:10:27.68 -00:31:02.8
06:58:26.17 -00:35:49.9
07:05:41.37 +00:53:11.5
07:13:12.96 +01:58:09.4
07:11:22.57 -01:09:07.0
07:03:37.07 -00:12:39.1
07:18:00.93 -01:12:31.8
06:56:30.39 -01:05:52.3
06:50:54.72 -00:02:41.4
07:10:27.43 -01:29:57.0
07:12:55.05 -01:57:59.6
07:15:07.58 +02:26:31.9
06:56:27.67 -01:27:43.2
07:18:21.30 -00:48:11.5
07:05:26.28 +01:29:35.0
06:48:21.58 +01:48:27.9
07:16:40.64 -01:23:41.7
06:49:11.62 +02:03:30.1
07:04:51.78 -00:22:11.6
07:06:20.25 +02:30:43.9
07:10:07.72 -02:09:54.0
06:42:18.78 +02:11:13.2
07:09:05.12 +01:56:10.4
06:48:10.05 -01:11:54.0
07:20:34.20 -00:45:30.2
07:10:55.26 -00:54:17.3
07:11:30.41 +00:31:16.9
06:55:37.79 +02:46:12.4
07:18:11.59 +02:33:20.1
06:45:04.68 +02:16:56.8
07:13:59.68 -00:06:57.6
07:01:31.08 -00:10:46.0
07:11:04.92 +01:22:09.1
06:49:31.20 +01:58:00.6
07:08:17.08 -00:08:18.5
07:16:12.26 -00:07:08.2
06:55:54.52 +02:54:12.4
06:35:13.38 -04:56:45.4
06:58:12.09 +01:19:08.9
06:54:40.05 +01:28:17.8
07:21:32.43 -00:16:17.2
06:58:39.27 -01:55:22.2
07:10:12.72 +01:37:53.5
06:55:20.64 +02:36:44.0
07:12:50.13 +01:20:16.7
07:10:59.27 -02:27:10.6
07:05:57.89 +02:49:16.7
06:54:41.21 -02:07:03.7
07:18:12.11 -02:02:25.6
07:05:15.75 +00:02:26.7
07:10:39.38 +00:54:03.6
07:08:25.07 +02:46:18.0
07:18:48.77 -01:43:45.9
07:08:21.83 -02:47:11.8
07:04:11.72 -01:14:21.1
07:05:38.92 -00:02:18.2
07:10:09.29 +00:56:13.2
07:00:52.11 +00:11:59.2
07:05:18.14 -01:22:58.9
06:58:57.13 -03:00:42.3
07:06:31.79 +02:11:35.5
07:11:19.89 -02:24:45.1
06:57:47.78 -01:31:07.2
06:44:25.06 +01:59:02.4
07:07:26.07 -01:50:44.5
07:14:00.58 -01:15:32.7
07:10:36.57 +00:49:12.4
06:48:15.68 +01:46:15.9
06:40:30.57 -01:04:42.8
06:42:42.58 +03:10:33.7
06:53:39.85 +01:30:57.2
06:53:50.91 -00:03:51.8
07:10:14.51 +02:07:07.6
06:48:50.65 -00:08:32.1
07:22:20.08 -01:09:42.1
07:18:23.32 +01:03:40.2
07:14:59.24 -01:45:23.7
07:09:20.73 +02:38:44.8
07:01:19.21 -03:06:43.4
07:04:18.50 -03:01:59.9
07:18:41.69 +01:11:02.7
07:04:51.44 -02:16:54.6
07:02:39.71 +01:10:07.4
07:04:54.75 +00:11:37.4
06:44:07.48 +03:13:06.7
06:52:49.53 +03:05:07.6
07:01:28.73 -01:08:32.7
07:12:56.34 +02:36:38.9
07:18:29.97 -00:11:37.0
07:01:04.49 +00:15:12.0
07:13:59.16 -01:53:58.4
07:16:05.29 +01:51:25.9
07:05:14.72 +00:02:12.7
07:16:21.46 +00:55:10.1
06:43:50.99 +01:35:56.1
06:59:40.61 -00:39:47.8
06:57:42.75 +01:19:13.5
07:12:57.03 +00:52:08.2
07:19:25.60 -02:06:13.4
07:20:50.44 -00:51:22.6
06:44:36.57 +01:45:26.7
07:01:14.63 +00:57:27.1
06:48:30.76 +00:57:44.2
06:34:30.30 +03:00:43.6
06:53:36.83 -02:31:46.9
06:48:35.75 -00:00:05.1
07:05:33.88 +02:07:16.9
07:04:46.70 +02:30:40.5
07:03:36.97 +02:37:09.5
06:56:49.13 +00:46:32.2
07:02:18.29 -02:01:26.0
07:04:16.83 -03:01:34.4
06:46:09.14 +02:40:03.6
07:14:45.41 -01:22:50.9
07:07:06.99 +01:39:59.7
06:42:42.37 -01:42:36.7
06:55:03.35 -01:02:51.2
07:06:07.44 -01:56:14.6
06:58:03.77 -00:47:09.0
06:30:03.32 +01:18:34.6
06:37:16.33 +03:08:55.4
07:10:42.79 -01:49:36.7
06:52:18.93 +03:03:40.2
07:06:45.79 -01:30:48.7
06:58:20.22 -00:33:16.9
06:49:07.36 -01:40:18.0
07:11:32.72 -01:56:46.4
07:15:39.68 -00:49:28.5
06:57:55.61 -00:57:57.2
07:05:20.65 +02:45:55.3
07:11:17.16 -01:29:12.8
06:45:39.00 +00:19:46.3
07:18:45.41 +02:22:33.7
07:08:30.79 +01:18:17.1
06:44:56.96 +01:18:44.4
07:02:49.63 -03:11:35.6
06:45:39.11 +02:45:21.6
07:00:38.82 -01:30:48.4
06:26:39.11 +00:26:39.0
06:59:44.36 -01:15:43.1
06:46:50.95 +01:18:08.0
07:13:40.87 -01:01:27.1
06:56:11.85 -01:22:24.0
06:49:56.16 -02:17:04.6
06:59:01.10 -02:36:01.4
07:05:49.37 +02:34:30.1
07:06:29.13 +02:03:03.8
06:55:19.17 +01:47:08.3
06:54:39.55 +02:38:00.0
06:59:35.85 -00:50:16.2
06:45:54.21 -00:09:38.1
07:08:46.25 -02:21:30.9
06:25:55.34 -00:53:21.7
06:50:59.68 +00:13:38.4
07:08:04.63 -01:43:42.0
06:45:33.85 -00:26:17.9
07:17:33.59 -01:43:04.5
06:54:39.28 +00:12:14.0
07:01:18.64 -03:25:50.7
07:11:20.26 +01:36:57.3
07:14:29.98 +01:49:07.0
06:54:26.46 +02:55:32.2
07:21:50.20 +00:09:22.6
06:55:16.06 +00:20:58.4
07:04:51.69 -02:12:04.6
07:06:54.27 +02:10:48.7
07:03:12.32 +01:32:44.2
06:56:54.24 +00:54:12.9
06:44:49.09 +01:46:41.0
06:49:54.82 +02:12:16.6
07:09:21.74 +01:07:27.4
06:59:00.81 +00:17:55.9
06:44:50.93 +01:05:44.2
07:11:38.36 +01:05:43.8
07:02:37.68 -01:54:04.8
07:09:56.82 -00:13:56.2
06:52:17.87 -03:21:57.5
06:48:57.15 -03:30:59.7
07:13:48.52 +02:30:38.5
07:01:47.31 -00:22:58.6
06:53:47.99 +00:29:47.2
07:07:03.77 -02:21:49.1
07:08:58.14 -02:02:45.9
06:30:01.86 -04:18:05.8
06:56:38.14 +00:32:04.1
06:38:19.80 +02:06:04.5
07:17:28.21 -01:37:00.1
07:07:24.37 -01:20:26.7
07:03:10.94 +01:19:42.5
07:03:46.12 -02:09:36.6
06:47:10.48 +02:54:02.2
07:12:25.57 +01:03:06.8
06:50:41.60 -00:31:45.7
06:46:32.69 -01:51:14.0
07:20:15.60 -02:00:46.4
06:47:16.50 +00:24:40.5
06:44:36.82 +00:59:54.2
07:02:21.27 -03:20:49.8
06:58:19.95 +02:48:59.0
06:42:20.84 +02:27:50.2
06:30:07.15 -02:39:48.6
06:59:42.47 +00:17:26.2
07:02:13.85 -00:12:25.2
07:14:24.74 +01:01:59.9
07:09:37.95 -00:01:19.0
07:05:47.91 +00:29:01.2
06:49:32.34 +01:56:36.0
07:01:02.14 +01:28:24.6
07:10:10.11 -00:03:48.8
07:02:55.80 -02:02:38.7
06:49:09.02 -01:39:04.2
06:46:17.59 +02:25:32.7
07:09:36.62 +01:42:30.9
06:47:59.75 -01:20:55.3
06:55:56.43 +02:39:55.9
06:55:11.97 +00:56:23.8
07:21:37.21 +00:28:48.2
07:09:27.00 -01:59:51.6
06:59:56.94 +02:16:59.9
06:53:43.69 -01:58:44.8
07:15:33.21 -01:08:35.0
07:07:06.88 +01:52:33.3
07:04:33.37 +01:07:10.0
06:49:46.20 -00:13:26.0
06:55:50.82 -02:12:27.9
07:17:57.96 +00:42:48.4
06:52:54.99 -02:58:59.1
06:33:52.92 -01:27:14.8
07:19:46.39 +00:48:05.1
06:58:48.13 -00:36:48.6
07:02:14.33 -00:35:02.5
06:49:21.58 +01:13:44.4
06:52:45.77 +01:05:34.7
07:04:20.04 +00:50:07.5
06:54:03.48 +02:06:09.3
06:58:34.29 -01:38:14.7
07:08:21.93 +01:09:06.7
06:37:27.75 +03:09:08.7
06:54:37.42 +02:24:26.8
07:08:49.41 -00:04:35.3
07:16:42.04 +02:29:03.9
07:03:54.33 -00:57:01.3
06:46:31.40 +01:08:37.5
07:00:29.10 +02:41:10.2
07:10:51.48 +00:26:29.0
07:00:16.18 +01:37:06.9
06:29:58.07 +03:04:34.2
06:57:12.94 -00:34:47.9
06:52:56.47 -02:22:53.3
07:18:57.19 -00:43:48.7
06:55:16.01 +01:54:57.3
07:13:00.83 -00:32:50.3
06:56:17.57 +01:28:36.3
07:11:46.26 +01:10:53.3
07:01:11.28 -00:44:18.2
06:43:53.97 +01:01:53.6
07:00:17.01 +01:41:49.3
06:51:47.51 +02:22:37.7
07:04:36.28 +02:03:16.2
06:59:46.73 -02:22:11.0
06:48:51.45 +02:00:14.8
06:49:31.33 +02:02:03.4
06:41:26.95 -01:17:39.5
06:45:26.37 -00:11:50.4
07:00:20.28 +01:48:26.0
06:45:59.16 +01:25:34.3
07:04:22.61 +00:59:50.4
06:55:29.83 -00:58:39.6
07:00:26.60 -00:13:24.1
06:56:35.73 -03:00:19.8
07:18:26.98 +00:26:42.9
06:52:13.49 -00:32:56.1
06:47:18.55 +02:46:09.0
07:16:03.24 -00:40:40.0
07:10:31.35 -00:55:58.4
07:14:36.80 -01:22:24.8
06:47:07.64 +01:46:45.3
07:11:30.95 +02:07:35.0
07:11:29.19 +00:13:44.9
07:14:48.01 +01:49:34.7
07:21:14.52 -01:19:48.9
06:58:04.84 +00:51:02.8
07:19:47.36 -00:02:48.7
07:17:34.67 +00:34:44.7
07:02:55.62 +02:43:38.3
07:05:01.79 +01:30:35.3
07:06:55.30 +00:27:40.6
07:14:15.01 +02:36:26.0
07:08:43.48 +01:22:16.7
06:46:49.53 +01:25:39.2
06:54:09.37 +01:41:21.1
07:13:34.41 +01:59:23.2
07:15:57.43 +02:41:29.0
06:49:40.20 -01:56:05.1
07:11:50.34 +01:30:56.8
06:47:02.72 +03:07:55.0
07:07:15.29 -02:45:48.6
07:16:43.51 +01:09:10.0
07:11:50.22 +01:54:46.4
06:55:38.36 +01:31:47.4
07:13:12.67 +01:29:20.3
07:18:50.08 -00:32:54.1
07:14:33.98 +01:07:26.5
06:58:36.41 -00:17:14.6
06:51:42.83 -01:56:08.2
07:21:35.99 +00:47:41.0
07:09:18.35 +00:20:29.3
06:53:35.87 +00:59:54.2
06:52:02.80 +01:24:02.6
06:59:00.28 -01:14:43.0
06:59:25.54 +01:32:51.5
07:03:53.68 +01:24:54.1
07:08:24.38 +01:25:13.8
06:48:57.56 +02:22:03.5
07:05:44.55 +00:49:31.5
06:50:45.69 -01:50:53.0
07:04:40.26 -01:02:14.9
07:11:19.12 -00:54:11.8
07:02:02.52 -02:08:44.8
07:13:26.15 -00:17:23.7
07:11:51.77 +01:45:14.1
07:15:46.04 -02:39:24.6
07:20:16.54 +01:20:10.0
07:05:41.63 +02:40:14.3
07:15:31.52 +02:29:20.0
06:58:19.57 -01:55:22.2
06:37:41.06 -03:18:49.6
06:41:48.67 +01:02:03.6
07:13:50.86 +01:53:48.9
06:56:25.48 +00:50:44.7
07:02:44.61 +02:16:17.0
06:39:07.96 +00:42:22.1
07:15:08.76 +00:57:28.1
07:11:40.10 -00:09:33.5
06:40:00.34 -01:07:11.8
07:11:21.13 +00:51:01.2
07:00:01.82 +00:36:59.6
07:00:33.00 -02:10:37.1
07:05:37.67 +02:21:34.8
06:48:20.06 +02:20:54.5
06:56:20.94 -02:49:04.9
06:54:02.36 -01:31:55.2
06:58:30.49 +00:42:34.4
06:45:55.43 +01:52:11.9
06:49:27.90 -03:07:23.4
06:21:42.58 -05:20:48.0
06:27:01.43 -04:35:40.1
06:21:55.11 -04:30:37.2
06:24:28.44 -04:05:49.0
########### 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 ####
07:09:13.73 -02:21:30.2
07:06:47.77 -02:29:52.1
06:46:26.73 +00:59:01.5
07:02:38.04 -00:50:21.9
07:06:28.80 -02:56:50.2
06:46:22.32 +01:50:05.6
06:46:25.15 +01:49:06.0
06:44:06.85 -00:12:06.2
06:43:22.55 +02:17:18.7
06:50:17.33 +02:23:27.3
07:05:25.69 -00:15:24.7
07:02:13.97 -01:26:47.7
06:47:57.05 +02:21:35.4
06:37:46.58 +01:47:14.8
07:02:18.17 +01:30:39.3
07:09:29.63 -02:28:31.9
06:43:22.75 +01:54:53.9
07:18:59.78 -00:08:13.5
07:03:41.13 -02:10:56.7
07:07:26.39 +01:04:08.9
07:01:30.56 +00:16:28.3
07:02:25.57 -01:07:14.1
07:15:02.37 -01:57:47.6
07:06:11.37 +00:35:33.6
07:19:50.64 +00:15:40.1
06:46:19.51 -01:57:15.3
06:37:32.00 +01:46:25.8
07:01:58.24 -02:16:30.3
07:10:27.68 -00:31:02.8
06:58:26.17 -00:35:49.9
07:05:41.37 +00:53:11.5
07:13:12.96 +01:58:09.4
07:11:22.57 -01:09:07.0
07:03:37.07 -00:12:39.1
07:18:00.93 -01:12:31.8
06:56:30.39 -01:05:52.3
06:50:54.72 -00:02:41.4
07:10:27.43 -01:29:57.0
07:12:55.05 -01:57:59.6
07:15:07.58 +02:26:31.9
06:56:27.67 -01:27:43.2
07:18:21.30 -00:48:11.5
07:05:26.28 +01:29:35.0
06:48:21.58 +01:48:27.9
07:16:40.64 -01:23:41.7
06:49:11.62 +02:03:30.1
07:04:51.78 -00:22:11.6
07:06:20.25 +02:30:43.9
07:10:07.72 -02:09:54.0
06:42:18.78 +02:11:13.2
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07:01:31.08 -00:10:46.0
07:11:04.92 +01:22:09.1
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07:08:17.08 -00:08:18.5
07:16:12.26 -00:07:08.2
06:55:54.52 +02:54:12.4
06:35:13.38 -04:56:45.4
06:58:12.09 +01:19:08.9
06:54:40.05 +01:28:17.8
07:21:32.43 -00:16:17.2
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07:10:12.72 +01:37:53.5
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07:10:59.27 -02:27:10.6
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07:05:15.75 +00:02:26.7
07:10:39.38 +00:54:03.6
07:08:25.07 +02:46:18.0
07:18:48.77 -01:43:45.9
07:08:21.83 -02:47:11.8
07:04:11.72 -01:14:21.1
07:05:38.92 -00:02:18.2
07:10:09.29 +00:56:13.2
07:00:52.11 +00:11:59.2
07:05:18.14 -01:22:58.9
06:58:57.13 -03:00:42.3
07:06:31.79 +02:11:35.5
07:11:19.89 -02:24:45.1
06:57:47.78 -01:31:07.2
06:44:25.06 +01:59:02.4
07:07:26.07 -01:50:44.5
07:14:00.58 -01:15:32.7
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06:48:15.68 +01:46:15.9
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06:42:42.58 +03:10:33.7
06:53:39.85 +01:30:57.2
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07:10:14.51 +02:07:07.6
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07:01:19.21 -03:06:43.4
07:04:18.50 -03:01:59.9
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07:02:39.71 +01:10:07.4
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07:05:14.72 +00:02:12.7
07:16:21.46 +00:55:10.1
06:43:50.99 +01:35:56.1
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07:12:57.03 +00:52:08.2
07:19:25.60 -02:06:13.4
07:20:50.44 -00:51:22.6
06:44:36.57 +01:45:26.7
07:01:14.63 +00:57:27.1
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06:34:30.30 +03:00:43.6
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07:04:46.70 +02:30:40.5
07:03:36.97 +02:37:09.5
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07:02:18.29 -02:01:26.0
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07:06:07.44 -01:56:14.6
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07:06:45.79 -01:30:48.7
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07:02:49.63 -03:11:35.6
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07:00:38.82 -01:30:48.4
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07:13:40.87 -01:01:27.1
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06:59:01.10 -02:36:01.4
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07:08:46.25 -02:21:30.9
06:25:55.34 -00:53:21.7
06:50:59.68 +00:13:38.4
07:08:04.63 -01:43:42.0
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07:17:33.59 -01:43:04.5
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07:01:18.64 -03:25:50.7
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07:03:12.32 +01:32:44.2
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07:02:37.68 -01:54:04.8
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06:52:17.87 -03:21:57.5
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07:01:47.31 -00:22:58.6
06:53:47.99 +00:29:47.2
07:07:03.77 -02:21:49.1
07:08:58.14 -02:02:45.9
06:30:01.86 -04:18:05.8
06:56:38.14 +00:32:04.1
06:38:19.80 +02:06:04.5
07:17:28.21 -01:37:00.1
07:07:24.37 -01:20:26.7
07:03:10.94 +01:19:42.5
07:03:46.12 -02:09:36.6
06:47:10.48 +02:54:02.2
07:12:25.57 +01:03:06.8
06:50:41.60 -00:31:45.7
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07:20:15.60 -02:00:46.4
06:47:16.50 +00:24:40.5
06:44:36.82 +00:59:54.2
07:02:21.27 -03:20:49.8
06:58:19.95 +02:48:59.0
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06:30:07.15 -02:39:48.6
06:59:42.47 +00:17:26.2
07:02:13.85 -00:12:25.2
07:14:24.74 +01:01:59.9
07:09:37.95 -00:01:19.0
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06:49:32.34 +01:56:36.0
07:01:02.14 +01:28:24.6
07:10:10.11 -00:03:48.8
07:02:55.80 -02:02:38.7
06:49:09.02 -01:39:04.2
06:46:17.59 +02:25:32.7
07:09:36.62 +01:42:30.9
06:47:59.75 -01:20:55.3
06:55:56.43 +02:39:55.9
06:55:11.97 +00:56:23.8
07:21:37.21 +00:28:48.2
07:09:27.00 -01:59:51.6
06:59:56.94 +02:16:59.9
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07:15:33.21 -01:08:35.0
07:07:06.88 +01:52:33.3
07:04:33.37 +01:07:10.0
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07:17:57.96 +00:42:48.4
06:52:54.99 -02:58:59.1
06:33:52.92 -01:27:14.8
07:19:46.39 +00:48:05.1
06:58:48.13 -00:36:48.6
07:02:14.33 -00:35:02.5
06:49:21.58 +01:13:44.4
06:52:45.77 +01:05:34.7
07:04:20.04 +00:50:07.5
06:54:03.48 +02:06:09.3
06:58:34.29 -01:38:14.7
07:08:21.93 +01:09:06.7
06:37:27.75 +03:09:08.7
06:54:37.42 +02:24:26.8
07:08:49.41 -00:04:35.3
07:16:42.04 +02:29:03.9
07:03:54.33 -00:57:01.3
06:46:31.40 +01:08:37.5
07:00:29.10 +02:41:10.2
07:10:51.48 +00:26:29.0
07:00:16.18 +01:37:06.9
06:29:58.07 +03:04:34.2
06:57:12.94 -00:34:47.9
06:52:56.47 -02:22:53.3
07:18:57.19 -00:43:48.7
06:55:16.01 +01:54:57.3
07:13:00.83 -00:32:50.3
06:56:17.57 +01:28:36.3
07:11:46.26 +01:10:53.3
07:01:11.28 -00:44:18.2
06:43:53.97 +01:01:53.6
07:00:17.01 +01:41:49.3
06:51:47.51 +02:22:37.7
07:04:36.28 +02:03:16.2
06:59:46.73 -02:22:11.0
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06:49:31.33 +02:02:03.4
06:41:26.95 -01:17:39.5
06:45:26.37 -00:11:50.4
07:00:20.28 +01:48:26.0
06:45:59.16 +01:25:34.3
07:04:22.61 +00:59:50.4
06:55:29.83 -00:58:39.6
07:00:26.60 -00:13:24.1
06:56:35.73 -03:00:19.8
07:18:26.98 +00:26:42.9
06:52:13.49 -00:32:56.1
06:47:18.55 +02:46:09.0
07:16:03.24 -00:40:40.0
07:10:31.35 -00:55:58.4
07:14:36.80 -01:22:24.8
06:47:07.64 +01:46:45.3
07:11:30.95 +02:07:35.0
07:11:29.19 +00:13:44.9
07:14:48.01 +01:49:34.7
07:21:14.52 -01:19:48.9
06:58:04.84 +00:51:02.8
07:19:47.36 -00:02:48.7
07:17:34.67 +00:34:44.7
07:02:55.62 +02:43:38.3
07:05:01.79 +01:30:35.3
07:06:55.30 +00:27:40.6
07:14:15.01 +02:36:26.0
07:08:43.48 +01:22:16.7
06:46:49.53 +01:25:39.2
06:54:09.37 +01:41:21.1
07:13:34.41 +01:59:23.2
07:15:57.43 +02:41:29.0
06:49:40.20 -01:56:05.1
07:11:50.34 +01:30:56.8
06:47:02.72 +03:07:55.0
07:07:15.29 -02:45:48.6
07:16:43.51 +01:09:10.0
07:11:50.22 +01:54:46.4
06:55:38.36 +01:31:47.4
07:13:12.67 +01:29:20.3
07:18:50.08 -00:32:54.1
07:14:33.98 +01:07:26.5
06:58:36.41 -00:17:14.6
06:51:42.83 -01:56:08.2
07:21:35.99 +00:47:41.0
07:09:18.35 +00:20:29.3
06:53:35.87 +00:59:54.2
06:52:02.80 +01:24:02.6
06:59:00.28 -01:14:43.0
06:59:25.54 +01:32:51.5
07:03:53.68 +01:24:54.1
07:08:24.38 +01:25:13.8
06:48:57.56 +02:22:03.5
07:05:44.55 +00:49:31.5
06:50:45.69 -01:50:53.0
07:04:40.26 -01:02:14.9
07:11:19.12 -00:54:11.8
07:02:02.52 -02:08:44.8
07:13:26.15 -00:17:23.7
07:11:51.77 +01:45:14.1
07:15:46.04 -02:39:24.6
07:20:16.54 +01:20:10.0
07:05:41.63 +02:40:14.3
07:15:31.52 +02:29:20.0
06:58:19.57 -01:55:22.2
06:37:41.06 -03:18:49.6
06:41:48.67 +01:02:03.6
07:13:50.86 +01:53:48.9
06:56:25.48 +00:50:44.7
07:02:44.61 +02:16:17.0
06:39:07.96 +00:42:22.1
07:15:08.76 +00:57:28.1
07:11:40.10 -00:09:33.5
06:40:00.34 -01:07:11.8
07:11:21.13 +00:51:01.2
07:00:01.82 +00:36:59.6
07:00:33.00 -02:10:37.1
07:05:37.67 +02:21:34.8
06:48:20.06 +02:20:54.5
06:56:20.94 -02:49:04.9
06:54:02.36 -01:31:55.2
06:58:30.49 +00:42:34.4
06:45:55.43 +01:52:11.9
06:49:27.90 -03:07:23.4
07:17:31.31 +01:05:38.1
06:27:01.43 -04:35:40.1
06:41:59.31 -01:11:07.3
06:21:42.58 -05:20:48.0
07:08:45.38 +00:41:47.6
06:21:55.11 -04:30:37.2
06:24:28.44 -04:05:49.0
07:05:28.89 -02:00:10.0
###################################################################################
07:09:13.73 -02:21:30.2 -- not an asteroid (will add it to exclusion list)
07:06:47.77 -02:29:52.1 -- not an asteroid (will add it to exclusion list)
06:46:26.73 +00:59:01.5 -- not an asteroid (will add it to exclusion list)
07:02:38.04 -00:50:21.9 -- not an asteroid (will add it to exclusion list)
07:06:28.80 -02:56:50.2 -- not an asteroid (will add it to exclusion list)
06:46:22.32 +01:50:05.6 -- not an asteroid (will add it to exclusion list)
06:46:25.15 +01:49:06.0 -- not an asteroid (will add it to exclusion list)
06:44:06.85 -00:12:06.2 -- not an asteroid (will add it to exclusion list)
06:43:22.55 +02:17:18.7 -- not an asteroid (will add it to exclusion list)
06:50:17.33 +02:23:27.3 -- not an asteroid (will add it to exclusion list)
07:05:25.69 -00:15:24.7 -- not an asteroid (will add it to exclusion list)
07:02:13.97 -01:26:47.7 -- not an asteroid (will add it to exclusion list)
06:47:57.05 +02:21:35.4 -- not an asteroid (will add it to exclusion list)
06:37:46.58 +01:47:14.8 -- not an asteroid (will add it to exclusion list)
07:02:18.17 +01:30:39.3 -- not an asteroid (will add it to exclusion list)
07:09:29.63 -02:28:31.9 -- not an asteroid (will add it to exclusion list)
06:43:22.75 +01:54:53.9 -- not an asteroid (will add it to exclusion list)
07:18:59.78 -00:08:13.5 -- not an asteroid (will add it to exclusion list)
07:03:41.13 -02:10:56.7 -- not an asteroid (will add it to exclusion list)
07:07:26.39 +01:04:08.9 -- not an asteroid (will add it to exclusion list)
07:01:30.56 +00:16:28.3 -- not an asteroid (will add it to exclusion list)
07:02:25.57 -01:07:14.1 -- not an asteroid (will add it to exclusion list)
07:15:02.37 -01:57:47.6 -- not an asteroid (will add it to exclusion list)
07:06:11.37 +00:35:33.6 -- not an asteroid (will add it to exclusion list)
07:19:50.64 +00:15:40.1 -- not an asteroid (will add it to exclusion list)
06:46:19.51 -01:57:15.3 -- not an asteroid (will add it to exclusion list)
06:37:32.00 +01:46:25.8 -- not an asteroid (will add it to exclusion list)
07:01:58.24 -02:16:30.3 -- not an asteroid (will add it to exclusion list)
07:10:27.68 -00:31:02.8 -- not an asteroid (will add it to exclusion list)
06:58:26.17 -00:35:49.9 -- not an asteroid (will add it to exclusion list)
07:05:41.37 +00:53:11.5 -- not an asteroid (will add it to exclusion list)
07:13:12.96 +01:58:09.4 -- not an asteroid (will add it to exclusion list)
07:11:22.57 -01:09:07.0 -- not an asteroid (will add it to exclusion list)
07:03:37.07 -00:12:39.1 -- not an asteroid (will add it to exclusion list)
07:18:00.93 -01:12:31.8 -- not an asteroid (will add it to exclusion list)
06:56:30.39 -01:05:52.3 -- not an asteroid (will add it to exclusion list)
06:50:54.72 -00:02:41.4 -- not an asteroid (will add it to exclusion list)
07:10:27.43 -01:29:57.0 -- not an asteroid (will add it to exclusion list)
07:12:55.05 -01:57:59.6 -- not an asteroid (will add it to exclusion list)
07:15:07.58 +02:26:31.9 -- not an asteroid (will add it to exclusion list)
06:56:27.67 -01:27:43.2 -- not an asteroid (will add it to exclusion list)
07:18:21.30 -00:48:11.5 -- not an asteroid (will add it to exclusion list)
07:05:26.28 +01:29:35.0 -- not an asteroid (will add it to exclusion list)
06:48:21.58 +01:48:27.9 -- not an asteroid (will add it to exclusion list)
07:16:40.64 -01:23:41.7 -- not an asteroid (will add it to exclusion list)
06:49:11.62 +02:03:30.1 -- not an asteroid (will add it to exclusion list)
07:04:51.78 -00:22:11.6 -- not an asteroid (will add it to exclusion list)
07:06:20.25 +02:30:43.9 -- not an asteroid (will add it to exclusion list)
07:10:07.72 -02:09:54.0 -- not an asteroid (will add it to exclusion list)
06:42:18.78 +02:11:13.2 -- not an asteroid (will add it to exclusion list)
07:09:05.12 +01:56:10.4 -- not an asteroid (will add it to exclusion list)
06:48:10.05 -01:11:54.0 -- not an asteroid (will add it to exclusion list)
07:20:34.20 -00:45:30.2 -- not an asteroid (will add it to exclusion list)
07:10:55.26 -00:54:17.3 -- not an asteroid (will add it to exclusion list)
07:11:30.41 +00:31:16.9 -- not an asteroid (will add it to exclusion list)
06:55:37.79 +02:46:12.4 -- not an asteroid (will add it to exclusion list)
07:18:11.59 +02:33:20.1 -- not an asteroid (will add it to exclusion list)
06:45:04.68 +02:16:56.8 -- not an asteroid (will add it to exclusion list)
07:13:59.68 -00:06:57.6 -- not an asteroid (will add it to exclusion list)
07:01:31.08 -00:10:46.0 -- not an asteroid (will add it to exclusion list)
07:11:04.92 +01:22:09.1 -- not an asteroid (will add it to exclusion list)
06:49:31.20 +01:58:00.6 -- not an asteroid (will add it to exclusion list)
07:08:17.08 -00:08:18.5 -- not an asteroid (will add it to exclusion list)
07:16:12.26 -00:07:08.2 -- not an asteroid (will add it to exclusion list)
06:55:54.52 +02:54:12.4 -- not an asteroid (will add it to exclusion list)
06:35:13.38 -04:56:45.4 -- not an asteroid (will add it to exclusion list)
06:58:12.09 +01:19:08.9 -- not an asteroid (will add it to exclusion list)
06:54:40.05 +01:28:17.8 -- not an asteroid (will add it to exclusion list)
07:21:32.43 -00:16:17.2 -- not an asteroid (will add it to exclusion list)
06:58:39.27 -01:55:22.2 -- not an asteroid (will add it to exclusion list)
07:10:12.72 +01:37:53.5 -- not an asteroid (will add it to exclusion list)
06:55:20.64 +02:36:44.0 -- not an asteroid (will add it to exclusion list)
07:12:50.13 +01:20:16.7 -- not an asteroid (will add it to exclusion list)
07:10:59.27 -02:27:10.6 -- not an asteroid (will add it to exclusion list)
07:05:57.89 +02:49:16.7 -- not an asteroid (will add it to exclusion list)
06:54:41.21 -02:07:03.7 -- not an asteroid (will add it to exclusion list)
07:18:12.11 -02:02:25.6 -- not an asteroid (will add it to exclusion list)
07:05:15.75 +00:02:26.7 -- not an asteroid (will add it to exclusion list)
07:10:39.38 +00:54:03.6 -- not an asteroid (will add it to exclusion list)
07:08:25.07 +02:46:18.0 -- not an asteroid (will add it to exclusion list)
07:18:48.77 -01:43:45.9 -- not an asteroid (will add it to exclusion list)
07:08:21.83 -02:47:11.8 -- not an asteroid (will add it to exclusion list)
07:04:11.72 -01:14:21.1 -- not an asteroid (will add it to exclusion list)
07:05:38.92 -00:02:18.2 -- not an asteroid (will add it to exclusion list)
07:10:09.29 +00:56:13.2 -- not an asteroid (will add it to exclusion list)
07:00:52.11 +00:11:59.2 -- not an asteroid (will add it to exclusion list)
07:05:18.14 -01:22:58.9 -- not an asteroid (will add it to exclusion list)
06:58:57.13 -03:00:42.3 -- not an asteroid (will add it to exclusion list)
07:06:31.79 +02:11:35.5 -- not an asteroid (will add it to exclusion list)
07:11:19.89 -02:24:45.1 -- not an asteroid (will add it to exclusion list)
06:57:47.78 -01:31:07.2 -- not an asteroid (will add it to exclusion list)
06:44:25.06 +01:59:02.4 -- not an asteroid (will add it to exclusion list)
07:07:26.07 -01:50:44.5 -- not an asteroid (will add it to exclusion list)
07:14:00.58 -01:15:32.7 -- not an asteroid (will add it to exclusion list)
07:10:36.57 +00:49:12.4 -- not an asteroid (will add it to exclusion list)
06:48:15.68 +01:46:15.9 -- not an asteroid (will add it to exclusion list)
06:40:30.57 -01:04:42.8 -- not an asteroid (will add it to exclusion list)
06:42:42.58 +03:10:33.7 -- not an asteroid (will add it to exclusion list)
06:53:39.85 +01:30:57.2 -- not an asteroid (will add it to exclusion list)
06:53:50.91 -00:03:51.8 -- not an asteroid (will add it to exclusion list)
07:10:14.51 +02:07:07.6 -- not an asteroid (will add it to exclusion list)
06:48:50.65 -00:08:32.1 -- not an asteroid (will add it to exclusion list)
07:22:20.08 -01:09:42.1 -- not an asteroid (will add it to exclusion list)
07:18:23.32 +01:03:40.2 -- not an asteroid (will add it to exclusion list)
07:14:59.24 -01:45:23.7 -- not an asteroid (will add it to exclusion list)
07:09:20.73 +02:38:44.8 -- not an asteroid (will add it to exclusion list)
07:01:19.21 -03:06:43.4 -- not an asteroid (will add it to exclusion list)
07:04:18.50 -03:01:59.9 -- not an asteroid (will add it to exclusion list)
07:18:41.69 +01:11:02.7 -- not an asteroid (will add it to exclusion list)
07:04:51.44 -02:16:54.6 -- not an asteroid (will add it to exclusion list)
07:02:39.71 +01:10:07.4 -- not an asteroid (will add it to exclusion list)
07:04:54.75 +00:11:37.4 -- not an asteroid (will add it to exclusion list)
06:44:07.48 +03:13:06.7 -- not an asteroid (will add it to exclusion list)
06:52:49.53 +03:05:07.6 -- not an asteroid (will add it to exclusion list)
07:01:28.73 -01:08:32.7 -- not an asteroid (will add it to exclusion list)
07:12:56.34 +02:36:38.9 -- not an asteroid (will add it to exclusion list)
07:18:29.97 -00:11:37.0 -- not an asteroid (will add it to exclusion list)
07:01:04.49 +00:15:12.0 -- not an asteroid (will add it to exclusion list)
07:13:59.16 -01:53:58.4 -- not an asteroid (will add it to exclusion list)
07:16:05.29 +01:51:25.9 -- not an asteroid (will add it to exclusion list)
07:05:14.72 +00:02:12.7 -- not an asteroid (will add it to exclusion list)
07:16:21.46 +00:55:10.1 -- not an asteroid (will add it to exclusion list)
06:43:50.99 +01:35:56.1 -- not an asteroid (will add it to exclusion list)
06:59:40.61 -00:39:47.8 -- not an asteroid (will add it to exclusion list)
06:57:42.75 +01:19:13.5 -- not an asteroid (will add it to exclusion list)
07:12:57.03 +00:52:08.2 -- not an asteroid (will add it to exclusion list)
07:19:25.60 -02:06:13.4 -- not an asteroid (will add it to exclusion list)
07:20:50.44 -00:51:22.6 -- not an asteroid (will add it to exclusion list)
06:44:36.57 +01:45:26.7 -- not an asteroid (will add it to exclusion list)
07:01:14.63 +00:57:27.1 -- not an asteroid (will add it to exclusion list)
06:48:30.76 +00:57:44.2 -- not an asteroid (will add it to exclusion list)
06:34:30.30 +03:00:43.6 -- not an asteroid (will add it to exclusion list)
06:53:36.83 -02:31:46.9 -- not an asteroid (will add it to exclusion list)
06:48:35.75 -00:00:05.1 -- not an asteroid (will add it to exclusion list)
07:05:33.88 +02:07:16.9 -- not an asteroid (will add it to exclusion list)
07:04:46.70 +02:30:40.5 -- not an asteroid (will add it to exclusion list)
07:03:36.97 +02:37:09.5 -- not an asteroid (will add it to exclusion list)
06:56:49.13 +00:46:32.2 -- not an asteroid (will add it to exclusion list)
07:02:18.29 -02:01:26.0 -- not an asteroid (will add it to exclusion list)
07:04:16.83 -03:01:34.4 -- not an asteroid (will add it to exclusion list)
06:46:09.14 +02:40:03.6 -- not an asteroid (will add it to exclusion list)
07:14:45.41 -01:22:50.9 -- not an asteroid (will add it to exclusion list)
07:07:06.99 +01:39:59.7 -- not an asteroid (will add it to exclusion list)
06:42:42.37 -01:42:36.7 -- not an asteroid (will add it to exclusion list)
06:55:03.35 -01:02:51.2 -- not an asteroid (will add it to exclusion list)
07:06:07.44 -01:56:14.6 -- not an asteroid (will add it to exclusion list)
06:58:03.77 -00:47:09.0 -- not an asteroid (will add it to exclusion list)
06:30:03.32 +01:18:34.6 -- not an asteroid (will add it to exclusion list)
06:37:16.33 +03:08:55.4 -- not an asteroid (will add it to exclusion list)
07:10:42.79 -01:49:36.7 -- not an asteroid (will add it to exclusion list)
06:52:18.93 +03:03:40.2 -- not an asteroid (will add it to exclusion list)
07:06:45.79 -01:30:48.7 -- not an asteroid (will add it to exclusion list)
06:58:20.22 -00:33:16.9 -- not an asteroid (will add it to exclusion list)
06:49:07.36 -01:40:18.0 -- not an asteroid (will add it to exclusion list)
07:11:32.72 -01:56:46.4 -- not an asteroid (will add it to exclusion list)
07:15:39.68 -00:49:28.5 -- not an asteroid (will add it to exclusion list)
06:57:55.61 -00:57:57.2 -- not an asteroid (will add it to exclusion list)
07:05:20.65 +02:45:55.3 -- not an asteroid (will add it to exclusion list)
07:11:17.16 -01:29:12.8 -- not an asteroid (will add it to exclusion list)
06:45:39.00 +00:19:46.3 -- not an asteroid (will add it to exclusion list)
07:18:45.41 +02:22:33.7 -- not an asteroid (will add it to exclusion list)
07:08:30.79 +01:18:17.1 -- not an asteroid (will add it to exclusion list)
06:44:56.96 +01:18:44.4 -- not an asteroid (will add it to exclusion list)
07:02:49.63 -03:11:35.6 -- not an asteroid (will add it to exclusion list)
06:45:39.11 +02:45:21.6 -- not an asteroid (will add it to exclusion list)
07:00:38.82 -01:30:48.4 -- not an asteroid (will add it to exclusion list)
06:26:39.11 +00:26:39.0 -- not an asteroid (will add it to exclusion list)
06:59:44.36 -01:15:43.1 -- not an asteroid (will add it to exclusion list)
06:46:50.95 +01:18:08.0 -- not an asteroid (will add it to exclusion list)
07:13:40.87 -01:01:27.1 -- not an asteroid (will add it to exclusion list)
06:56:11.85 -01:22:24.0 -- not an asteroid (will add it to exclusion list)
06:49:56.16 -02:17:04.6 -- not an asteroid (will add it to exclusion list)
06:59:01.10 -02:36:01.4 -- not an asteroid (will add it to exclusion list)
07:05:49.37 +02:34:30.1 -- not an asteroid (will add it to exclusion list)
07:06:29.13 +02:03:03.8 -- not an asteroid (will add it to exclusion list)
06:55:19.17 +01:47:08.3 -- not an asteroid (will add it to exclusion list)
06:54:39.55 +02:38:00.0 -- not an asteroid (will add it to exclusion list)
06:59:35.85 -00:50:16.2 -- not an asteroid (will add it to exclusion list)
06:45:54.21 -00:09:38.1 -- not an asteroid (will add it to exclusion list)
07:08:46.25 -02:21:30.9 -- not an asteroid (will add it to exclusion list)
06:25:55.34 -00:53:21.7 -- not an asteroid (will add it to exclusion list)
06:50:59.68 +00:13:38.4 -- not an asteroid (will add it to exclusion list)
07:08:04.63 -01:43:42.0 -- not an asteroid (will add it to exclusion list)
06:45:33.85 -00:26:17.9 -- not an asteroid (will add it to exclusion list)
07:17:33.59 -01:43:04.5 -- not an asteroid (will add it to exclusion list)
06:54:39.28 +00:12:14.0 -- not an asteroid (will add it to exclusion list)
07:01:18.64 -03:25:50.7 -- not an asteroid (will add it to exclusion list)
07:11:20.26 +01:36:57.3 -- not an asteroid (will add it to exclusion list)
07:14:29.98 +01:49:07.0 -- not an asteroid (will add it to exclusion list)
06:54:26.46 +02:55:32.2 -- not an asteroid (will add it to exclusion list)
07:21:50.20 +00:09:22.6 -- not an asteroid (will add it to exclusion list)
06:55:16.06 +00:20:58.4 -- not an asteroid (will add it to exclusion list)
07:04:51.69 -02:12:04.6 -- not an asteroid (will add it to exclusion list)
07:06:54.27 +02:10:48.7 -- not an asteroid (will add it to exclusion list)
07:03:12.32 +01:32:44.2 -- not an asteroid (will add it to exclusion list)
06:56:54.24 +00:54:12.9 -- not an asteroid (will add it to exclusion list)
06:44:49.09 +01:46:41.0 -- not an asteroid (will add it to exclusion list)
06:49:54.82 +02:12:16.6 -- not an asteroid (will add it to exclusion list)
07:09:21.74 +01:07:27.4 -- not an asteroid (will add it to exclusion list)
06:59:00.81 +00:17:55.9 -- not an asteroid (will add it to exclusion list)
06:44:50.93 +01:05:44.2 -- not an asteroid (will add it to exclusion list)
07:11:38.36 +01:05:43.8 -- not an asteroid (will add it to exclusion list)
07:02:37.68 -01:54:04.8 -- not an asteroid (will add it to exclusion list)
07:09:56.82 -00:13:56.2 -- not an asteroid (will add it to exclusion list)
06:52:17.87 -03:21:57.5 -- not an asteroid (will add it to exclusion list)
06:48:57.15 -03:30:59.7 -- not an asteroid (will add it to exclusion list)
07:13:48.52 +02:30:38.5 -- not an asteroid (will add it to exclusion list)
07:01:47.31 -00:22:58.6 -- not an asteroid (will add it to exclusion list)
06:53:47.99 +00:29:47.2 -- not an asteroid (will add it to exclusion list)
07:07:03.77 -02:21:49.1 -- not an asteroid (will add it to exclusion list)
07:08:58.14 -02:02:45.9 -- not an asteroid (will add it to exclusion list)
06:30:01.86 -04:18:05.8 -- not an asteroid (will add it to exclusion list)
06:56:38.14 +00:32:04.1 -- not an asteroid (will add it to exclusion list)
06:38:19.80 +02:06:04.5 -- not an asteroid (will add it to exclusion list)
07:17:28.21 -01:37:00.1 -- not an asteroid (will add it to exclusion list)
07:07:24.37 -01:20:26.7 -- not an asteroid (will add it to exclusion list)
07:03:10.94 +01:19:42.5 -- not an asteroid (will add it to exclusion list)
07:03:46.12 -02:09:36.6 -- not an asteroid (will add it to exclusion list)
06:47:10.48 +02:54:02.2 -- not an asteroid (will add it to exclusion list)
07:12:25.57 +01:03:06.8 -- not an asteroid (will add it to exclusion list)
06:50:41.60 -00:31:45.7 -- not an asteroid (will add it to exclusion list)
06:46:32.69 -01:51:14.0 -- not an asteroid (will add it to exclusion list)
07:20:15.60 -02:00:46.4 -- not an asteroid (will add it to exclusion list)
06:47:16.50 +00:24:40.5 -- not an asteroid (will add it to exclusion list)
06:44:36.82 +00:59:54.2 -- not an asteroid (will add it to exclusion list)
07:02:21.27 -03:20:49.8 -- not an asteroid (will add it to exclusion list)
06:58:19.95 +02:48:59.0 -- not an asteroid (will add it to exclusion list)
06:42:20.84 +02:27:50.2 -- not an asteroid (will add it to exclusion list)
06:30:07.15 -02:39:48.6 -- not an asteroid (will add it to exclusion list)
06:59:42.47 +00:17:26.2 -- not an asteroid (will add it to exclusion list)
07:02:13.85 -00:12:25.2 -- not an asteroid (will add it to exclusion list)
07:14:24.74 +01:01:59.9 -- not an asteroid (will add it to exclusion list)
07:09:37.95 -00:01:19.0 -- not an asteroid (will add it to exclusion list)
07:05:47.91 +00:29:01.2 -- not an asteroid (will add it to exclusion list)
06:49:32.34 +01:56:36.0 -- not an asteroid (will add it to exclusion list)
07:01:02.14 +01:28:24.6 -- not an asteroid (will add it to exclusion list)
07:10:10.11 -00:03:48.8 -- not an asteroid (will add it to exclusion list)
07:02:55.80 -02:02:38.7 -- not an asteroid (will add it to exclusion list)
06:49:09.02 -01:39:04.2 -- not an asteroid (will add it to exclusion list)
06:46:17.59 +02:25:32.7 -- not an asteroid (will add it to exclusion list)
07:09:36.62 +01:42:30.9 -- not an asteroid (will add it to exclusion list)
06:47:59.75 -01:20:55.3 -- not an asteroid (will add it to exclusion list)
06:55:56.43 +02:39:55.9 -- not an asteroid (will add it to exclusion list)
06:55:11.97 +00:56:23.8 -- not an asteroid (will add it to exclusion list)
07:21:37.21 +00:28:48.2 -- not an asteroid (will add it to exclusion list)
07:09:27.00 -01:59:51.6 -- not an asteroid (will add it to exclusion list)
06:59:56.94 +02:16:59.9 -- not an asteroid (will add it to exclusion list)
06:53:43.69 -01:58:44.8 -- not an asteroid (will add it to exclusion list)
07:15:33.21 -01:08:35.0 -- not an asteroid (will add it to exclusion list)
07:07:06.88 +01:52:33.3 -- not an asteroid (will add it to exclusion list)
07:04:33.37 +01:07:10.0 -- not an asteroid (will add it to exclusion list)
06:49:46.20 -00:13:26.0 -- not an asteroid (will add it to exclusion list)
06:55:50.82 -02:12:27.9 -- not an asteroid (will add it to exclusion list)
07:17:57.96 +00:42:48.4 -- not an asteroid (will add it to exclusion list)
06:52:54.99 -02:58:59.1 -- not an asteroid (will add it to exclusion list)
06:33:52.92 -01:27:14.8 -- not an asteroid (will add it to exclusion list)
07:19:46.39 +00:48:05.1 -- not an asteroid (will add it to exclusion list)
06:58:48.13 -00:36:48.6 -- not an asteroid (will add it to exclusion list)
07:02:14.33 -00:35:02.5 -- not an asteroid (will add it to exclusion list)
06:49:21.58 +01:13:44.4 -- not an asteroid (will add it to exclusion list)
06:52:45.77 +01:05:34.7 -- not an asteroid (will add it to exclusion list)
07:04:20.04 +00:50:07.5 -- not an asteroid (will add it to exclusion list)
06:54:03.48 +02:06:09.3 -- not an asteroid (will add it to exclusion list)
06:58:34.29 -01:38:14.7 -- not an asteroid (will add it to exclusion list)
07:08:21.93 +01:09:06.7 -- not an asteroid (will add it to exclusion list)
06:37:27.75 +03:09:08.7 -- not an asteroid (will add it to exclusion list)
06:54:37.42 +02:24:26.8 -- not an asteroid (will add it to exclusion list)
07:08:49.41 -00:04:35.3 -- not an asteroid (will add it to exclusion list)
07:16:42.04 +02:29:03.9 -- not an asteroid (will add it to exclusion list)
07:03:54.33 -00:57:01.3 -- not an asteroid (will add it to exclusion list)
06:46:31.40 +01:08:37.5 -- not an asteroid (will add it to exclusion list)
07:00:29.10 +02:41:10.2 -- not an asteroid (will add it to exclusion list)
07:10:51.48 +00:26:29.0 -- not an asteroid (will add it to exclusion list)
07:00:16.18 +01:37:06.9 -- not an asteroid (will add it to exclusion list)
06:29:58.07 +03:04:34.2 -- not an asteroid (will add it to exclusion list)
06:57:12.94 -00:34:47.9 -- not an asteroid (will add it to exclusion list)
06:52:56.47 -02:22:53.3 -- not an asteroid (will add it to exclusion list)
07:18:57.19 -00:43:48.7 -- not an asteroid (will add it to exclusion list)
06:55:16.01 +01:54:57.3 -- not an asteroid (will add it to exclusion list)
07:13:00.83 -00:32:50.3 -- not an asteroid (will add it to exclusion list)
06:56:17.57 +01:28:36.3 -- not an asteroid (will add it to exclusion list)
07:11:46.26 +01:10:53.3 -- not an asteroid (will add it to exclusion list)
07:01:11.28 -00:44:18.2 -- not an asteroid (will add it to exclusion list)
06:43:53.97 +01:01:53.6 -- not an asteroid (will add it to exclusion list)
07:00:17.01 +01:41:49.3 -- not an asteroid (will add it to exclusion list)
06:51:47.51 +02:22:37.7 -- not an asteroid (will add it to exclusion list)
07:04:36.28 +02:03:16.2 -- not an asteroid (will add it to exclusion list)
06:59:46.73 -02:22:11.0 -- not an asteroid (will add it to exclusion list)
06:48:51.45 +02:00:14.8 -- not an asteroid (will add it to exclusion list)
06:49:31.33 +02:02:03.4 -- not an asteroid (will add it to exclusion list)
06:41:26.95 -01:17:39.5 -- not an asteroid (will add it to exclusion list)
06:45:26.37 -00:11:50.4 -- not an asteroid (will add it to exclusion list)
07:00:20.28 +01:48:26.0 -- not an asteroid (will add it to exclusion list)
06:45:59.16 +01:25:34.3 -- not an asteroid (will add it to exclusion list)
07:04:22.61 +00:59:50.4 -- not an asteroid (will add it to exclusion list)
06:55:29.83 -00:58:39.6 -- not an asteroid (will add it to exclusion list)
07:00:26.60 -00:13:24.1 -- not an asteroid (will add it to exclusion list)
06:56:35.73 -03:00:19.8 -- not an asteroid (will add it to exclusion list)
07:18:26.98 +00:26:42.9 -- not an asteroid (will add it to exclusion list)
06:52:13.49 -00:32:56.1 -- not an asteroid (will add it to exclusion list)
06:47:18.55 +02:46:09.0 -- not an asteroid (will add it to exclusion list)
07:16:03.24 -00:40:40.0 -- not an asteroid (will add it to exclusion list)
07:10:31.35 -00:55:58.4 -- not an asteroid (will add it to exclusion list)
07:14:36.80 -01:22:24.8 -- not an asteroid (will add it to exclusion list)
06:47:07.64 +01:46:45.3 -- not an asteroid (will add it to exclusion list)
07:11:30.95 +02:07:35.0 -- not an asteroid (will add it to exclusion list)
07:11:29.19 +00:13:44.9 -- not an asteroid (will add it to exclusion list)
07:14:48.01 +01:49:34.7 -- not an asteroid (will add it to exclusion list)
07:21:14.52 -01:19:48.9 -- not an asteroid (will add it to exclusion list)
06:58:04.84 +00:51:02.8 -- not an asteroid (will add it to exclusion list)
07:19:47.36 -00:02:48.7 -- not an asteroid (will add it to exclusion list)
07:17:34.67 +00:34:44.7 -- not an asteroid (will add it to exclusion list)
07:02:55.62 +02:43:38.3 -- not an asteroid (will add it to exclusion list)
07:05:01.79 +01:30:35.3 -- not an asteroid (will add it to exclusion list)
07:06:55.30 +00:27:40.6 -- not an asteroid (will add it to exclusion list)
07:14:15.01 +02:36:26.0 -- not an asteroid (will add it to exclusion list)
07:08:43.48 +01:22:16.7 -- not an asteroid (will add it to exclusion list)
06:46:49.53 +01:25:39.2 -- not an asteroid (will add it to exclusion list)
06:54:09.37 +01:41:21.1 -- not an asteroid (will add it to exclusion list)
07:13:34.41 +01:59:23.2 -- not an asteroid (will add it to exclusion list)
07:15:57.43 +02:41:29.0 -- not an asteroid (will add it to exclusion list)
06:49:40.20 -01:56:05.1 -- not an asteroid (will add it to exclusion list)
07:11:50.34 +01:30:56.8 -- not an asteroid (will add it to exclusion list)
06:47:02.72 +03:07:55.0 -- not an asteroid (will add it to exclusion list)
07:07:15.29 -02:45:48.6 -- not an asteroid (will add it to exclusion list)
07:16:43.51 +01:09:10.0 -- not an asteroid (will add it to exclusion list)
07:11:50.22 +01:54:46.4 -- not an asteroid (will add it to exclusion list)
06:55:38.36 +01:31:47.4 -- not an asteroid (will add it to exclusion list)
07:13:12.67 +01:29:20.3 -- not an asteroid (will add it to exclusion list)
07:18:50.08 -00:32:54.1 -- not an asteroid (will add it to exclusion list)
07:14:33.98 +01:07:26.5 -- not an asteroid (will add it to exclusion list)
06:58:36.41 -00:17:14.6 -- not an asteroid (will add it to exclusion list)
06:51:42.83 -01:56:08.2 -- not an asteroid (will add it to exclusion list)
07:21:35.99 +00:47:41.0 -- not an asteroid (will add it to exclusion list)
07:09:18.35 +00:20:29.3 -- not an asteroid (will add it to exclusion list)
06:53:35.87 +00:59:54.2 -- not an asteroid (will add it to exclusion list)
06:52:02.80 +01:24:02.6 -- not an asteroid (will add it to exclusion list)
06:59:00.28 -01:14:43.0 -- not an asteroid (will add it to exclusion list)
06:59:25.54 +01:32:51.5 -- not an asteroid (will add it to exclusion list)
07:03:53.68 +01:24:54.1 -- not an asteroid (will add it to exclusion list)
07:08:24.38 +01:25:13.8 -- not an asteroid (will add it to exclusion list)
06:48:57.56 +02:22:03.5 -- not an asteroid (will add it to exclusion list)
07:05:44.55 +00:49:31.5 -- not an asteroid (will add it to exclusion list)
06:50:45.69 -01:50:53.0 -- not an asteroid (will add it to exclusion list)
07:04:40.26 -01:02:14.9 -- not an asteroid (will add it to exclusion list)
07:11:19.12 -00:54:11.8 -- not an asteroid (will add it to exclusion list)
07:02:02.52 -02:08:44.8 -- not an asteroid (will add it to exclusion list)
07:13:26.15 -00:17:23.7 -- not an asteroid (will add it to exclusion list)
07:11:51.77 +01:45:14.1 -- not an asteroid (will add it to exclusion list)
07:15:46.04 -02:39:24.6 -- not an asteroid (will add it to exclusion list)
07:20:16.54 +01:20:10.0 -- not an asteroid (will add it to exclusion list)
07:05:41.63 +02:40:14.3 -- not an asteroid (will add it to exclusion list)
07:15:31.52 +02:29:20.0 -- not an asteroid (will add it to exclusion list)
06:58:19.57 -01:55:22.2 -- not an asteroid (will add it to exclusion list)
06:37:41.06 -03:18:49.6 -- not an asteroid (will add it to exclusion list)
06:41:48.67 +01:02:03.6 -- not an asteroid (will add it to exclusion list)
07:13:50.86 +01:53:48.9 -- not an asteroid (will add it to exclusion list)
06:56:25.48 +00:50:44.7 -- not an asteroid (will add it to exclusion list)
07:02:44.61 +02:16:17.0 -- not an asteroid (will add it to exclusion list)
06:39:07.96 +00:42:22.1 -- not an asteroid (will add it to exclusion list)
07:15:08.76 +00:57:28.1 -- not an asteroid (will add it to exclusion list)
07:11:40.10 -00:09:33.5 -- not an asteroid (will add it to exclusion list)
06:40:00.34 -01:07:11.8 -- not an asteroid (will add it to exclusion list)
07:11:21.13 +00:51:01.2 -- not an asteroid (will add it to exclusion list)
07:00:01.82 +00:36:59.6 -- not an asteroid (will add it to exclusion list)
07:00:33.00 -02:10:37.1 -- not an asteroid (will add it to exclusion list)
07:05:37.67 +02:21:34.8 -- not an asteroid (will add it to exclusion list)
06:48:20.06 +02:20:54.5 -- not an asteroid (will add it to exclusion list)
06:56:20.94 -02:49:04.9 -- not an asteroid (will add it to exclusion list)
06:54:02.36 -01:31:55.2 -- not an asteroid (will add it to exclusion list)
06:58:30.49 +00:42:34.4 -- not an asteroid (will add it to exclusion list)
06:45:55.43 +01:52:11.9 -- not an asteroid (will add it to exclusion list)
06:49:27.90 -03:07:23.4 -- not an asteroid (will add it to exclusion list)
07:17:31.31 +01:05:38.1 -- not an asteroid (will add it to exclusion list)
06:27:01.43 -04:35:40.1 -- not an asteroid (will add it to exclusion list)
06:41:59.31 -01:11:07.3 -- not an asteroid (will add it to exclusion list)
06:21:42.58 -05:20:48.0 -- not an asteroid (will add it to exclusion list)
07:08:45.38 +00:41:47.6 -- not an asteroid (will add it to exclusion list)
06:21:55.11 -04:30:37.2 -- not an asteroid (will add it to exclusion list)
06:24:28.44 -04:05:49.0 -- not an asteroid (will add it to exclusion list)
07:05:28.89 -02:00:10.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:21:42.58 -05:20:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:55.11 -04:30:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:28.44 -04:05:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:55.34 -00:53:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:39.11 +00:26:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:01.43 -04:35:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:58.07 +03:04:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:01.86 -04:18:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:03.32 +01:18:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:07.15 -02:39:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:52.92 -01:27:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:30.30 +03:00:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:13.38 -04:56:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:16.33 +03:08:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:27.75 +03:09:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:32.00 +01:46:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:41.06 -03:18:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:46.58 +01:47:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:19.80 +02:06:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:07.96 +00:42:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:00.34 -01:07:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.57 -01:04:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.95 -01:17:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:48.67 +01:02:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:59.31 -01:11:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:18.78 +02:11:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:20.84 +02:27:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.37 -01:42:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.58 +03:10:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:22.55 +02:17:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:22.75 +01:54:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:50.99 +01:35:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:53.97 +01:01:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:06.85 -00:12:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:07.48 +03:13:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:25.06 +01:59:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.57 +01:45:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.82 +00:59:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:49.09 +01:46:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.93 +01:05:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:56.96 +01:18:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:04.68 +02:16:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:26.37 -00:11:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.85 -00:26:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.00 +00:19:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.11 +02:45:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.21 -00:09:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:55.43 +01:52:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:59.16 +01:25:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:09.14 +02:40:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:17.59 +02:25:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:19.51 -01:57:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:22.32 +01:50:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.15 +01:49:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:26.73 +00:59:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.40 +01:08:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.69 -01:51:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:49.53 +01:25:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:50.95 +01:18:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:02.72 +03:07:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:07.64 +01:46:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.48 +02:54:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:16.50 +00:24:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:18.55 +02:46:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:57.05 +02:21:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.75 -01:20:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:10.05 -01:11:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.68 +01:46:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:20.06 +02:20:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:21.58 +01:48:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:30.76 +00:57:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:35.75 -00:00:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:50.65 -00:08:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:51.45 +02:00:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:57.15 -03:30:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:57.56 +02:22:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.36 -01:40:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:09.02 -01:39:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:11.62 +02:03:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:21.58 +01:13:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:27.90 -03:07:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:31.20 +01:58:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:31.33 +02:02:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:32.34 +01:56:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:40.20 -01:56:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:46.20 -00:13:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:54.82 +02:12:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.16 -02:17:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:17.33 +02:23:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.60 -00:31:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:45.69 -01:50:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:54.72 -00:02:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.68 +00:13:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:42.83 -01:56:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:47.51 +02:22:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:02.80 +01:24:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:13.49 -00:32:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:17.87 -03:21:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:18.93 +03:03:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:45.77 +01:05:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:49.53 +03:05:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:54.99 -02:58:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:56.47 -02:22:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:35.87 +00:59:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.83 -02:31:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:39.85 +01:30:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.69 -01:58:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.99 +00:29:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:50.91 -00:03:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:02.36 -01:31:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:03.48 +02:06:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:09.37 +01:41:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:26.46 +02:55:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:37.42 +02:24:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.28 +00:12:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.55 +02:38:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:40.05 +01:28:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.21 -02:07:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.35 -01:02:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.97 +00:56:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:16.01 +01:54:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:16.06 +00:20:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:19.17 +01:47:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:20.64 +02:36:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:29.83 -00:58:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:37.79 +02:46:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:38.36 +01:31:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.82 -02:12:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:54.52 +02:54:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:56.43 +02:39:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:11.85 -01:22:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:17.57 +01:28:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:20.94 -02:49:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:25.48 +00:50:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:27.67 -01:27:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:30.39 -01:05:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:35.73 -03:00:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:38.14 +00:32:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:49.13 +00:46:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:54.24 +00:54:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.94 -00:34:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:42.75 +01:19:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.78 -01:31:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.61 -00:57:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:03.77 -00:47:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:04.84 +00:51:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:12.09 +01:19:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:19.57 -01:55:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:19.95 +02:48:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:20.22 -00:33:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:26.17 -00:35:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:30.49 +00:42:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.29 -01:38:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:36.41 -00:17:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.27 -01:55:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:48.13 -00:36:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.13 -03:00:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.28 -01:14:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.81 +00:17:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:01.10 -02:36:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:25.54 +01:32:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:35.85 -00:50:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.61 -00:39:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.47 +00:17:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:44.36 -01:15:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:46.73 -02:22:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:56.94 +02:16:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.82 +00:36:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:16.18 +01:37:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:17.01 +01:41:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:20.28 +01:48:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:26.60 -00:13:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:29.10 +02:41:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:33.00 -02:10:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:38.82 -01:30:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:52.11 +00:11:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:02.14 +01:28:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:04.49 +00:15:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:11.28 -00:44:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.63 +00:57:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:18.64 -03:25:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.21 -03:06:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:28.73 -01:08:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:30.56 +00:16:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:31.08 -00:10:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:47.31 -00:22:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:58.24 -02:16:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:02.52 -02:08:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:13.85 -00:12:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:13.97 -01:26:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.33 -00:35:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:18.17 +01:30:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:18.29 -02:01:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.27 -03:20:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:25.57 -01:07:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:37.68 -01:54:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:38.04 -00:50:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:39.71 +01:10:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:44.61 +02:16:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:49.63 -03:11:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:55.62 +02:43:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:55.80 -02:02:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:10.94 +01:19:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:12.32 +01:32:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.97 +02:37:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:37.07 -00:12:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:41.13 -02:10:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:46.12 -02:09:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:53.68 +01:24:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:54.33 -00:57:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:11.72 -01:14:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.83 -03:01:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:18.50 -03:01:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.04 +00:50:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:22.61 +00:59:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:33.37 +01:07:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:36.28 +02:03:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:40.26 -01:02:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:46.70 +02:30:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.44 -02:16:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.69 -02:12:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.78 -00:22:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:54.75 +00:11:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:01.79 +01:30:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.72 +00:02:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:15.75 +00:02:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.14 -01:22:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.65 +02:45:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:25.69 -00:15:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:26.28 +01:29:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:28.89 -02:00:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:33.88 +02:07:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:37.67 +02:21:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.92 -00:02:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.37 +00:53:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.63 +02:40:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:44.55 +00:49:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:47.91 +00:29:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:49.37 +02:34:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:57.89 +02:49:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:07.44 -01:56:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.37 +00:35:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:20.25 +02:30:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:28.80 -02:56:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:29.13 +02:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.79 +02:11:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.79 -01:30:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:47.77 -02:29:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.27 +02:10:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:55.30 +00:27:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:03.77 -02:21:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.88 +01:52:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.99 +01:39:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.29 -02:45:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.37 -01:20:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.07 -01:50:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.39 +01:04:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:04.63 -01:43:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:17.08 -00:08:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:21.83 -02:47:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:21.93 +01:09:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:24.38 +01:25:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:25.07 +02:46:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:30.79 +01:18:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.48 +01:22:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.38 +00:41:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:46.25 -02:21:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:49.41 -00:04:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:58.14 -02:02:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.12 +01:56:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.73 -02:21:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:18.35 +00:20:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.73 +02:38:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.74 +01:07:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:27.00 -01:59:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:29.63 -02:28:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:36.62 +01:42:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:37.95 -00:01:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:56.82 -00:13:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:07.72 -02:09:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:09.29 +00:56:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.11 -00:03:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:12.72 +01:37:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:14.51 +02:07:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:27.43 -01:29:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:27.68 -00:31:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:31.35 -00:55:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:36.57 +00:49:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:39.38 +00:54:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:42.79 -01:49:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:51.48 +00:26:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:55.26 -00:54:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:59.27 -02:27:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:04.92 +01:22:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:17.16 -01:29:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.12 -00:54:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.89 -02:24:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:20.26 +01:36:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:21.13 +00:51:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:22.57 -01:09:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:29.19 +00:13:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:30.41 +00:31:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:30.95 +02:07:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:32.72 -01:56:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:38.36 +01:05:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:40.10 -00:09:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:46.26 +01:10:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:50.22 +01:54:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:50.34 +01:30:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:51.77 +01:45:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:25.57 +01:03:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:50.13 +01:20:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:55.05 -01:57:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.34 +02:36:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:57.03 +00:52:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:00.83 -00:32:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:12.67 +01:29:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:12.96 +01:58:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:26.15 -00:17:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:34.41 +01:59:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:40.87 -01:01:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:48.52 +02:30:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:50.86 +01:53:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:59.16 -01:53:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:59.68 -00:06:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:00.58 -01:15:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:15.01 +02:36:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:24.74 +01:01:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:29.98 +01:49:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:33.98 +01:07:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:36.80 -01:22:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:45.41 -01:22:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:48.01 +01:49:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:59.24 -01:45:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:02.37 -01:57:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:07.58 +02:26:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:08.76 +00:57:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:31.52 +02:29:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:33.21 -01:08:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:39.68 -00:49:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:46.04 -02:39:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:57.43 +02:41:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.24 -00:40:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:05.29 +01:51:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:12.26 -00:07:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:21.46 +00:55:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:40.64 -01:23:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:42.04 +02:29:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:43.51 +01:09:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:28.21 -01:37:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.31 +01:05:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:33.59 -01:43:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:34.67 +00:34:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:57.96 +00:42:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:00.93 -01:12:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:11.59 +02:33:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:12.11 -02:02:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:21.30 -00:48:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:23.32 +01:03:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:26.98 +00:26:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:29.97 -00:11:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:41.69 +01:11:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:45.41 +02:22:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:48.77 -01:43:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:50.08 -00:32:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:57.19 -00:43:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:59.78 -00:08:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:25.60 -02:06:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:46.39 +00:48:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:47.36 -00:02:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:50.64 +00:15:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:15.60 -02:00:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:16.54 +01:20:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:34.20 -00:45:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:50.44 -00:51:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:14.52 -01:19:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:32.43 -00:16:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:35.99 +00:47:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:37.21 +00:28:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:50.20 +00:09:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:20.08 -01:09:42.1 -- 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)
06:21:42.58 -05:20:48.0 -- not a known variable star
06:21:55.11 -04:30:37.2 -- not a known variable star
06:24:28.44 -04:05:49.0 -- not a known variable star
06:25:55.34 -00:53:21.7 -- not a known variable star
06:26:39.11 +00:26:39.0 -- not a known variable star
06:27:01.43 -04:35:40.1 -- a known variable star
06:29:58.07 +03:04:34.2 -- not a known variable star
06:30:01.86 -04:18:05.8 -- not a known variable star
06:30:03.32 +01:18:34.6 -- a known variable star
06:30:07.15 -02:39:48.6 -- not a known variable star
06:33:52.92 -01:27:14.8 -- a known variable star
06:34:30.30 +03:00:43.6 -- not a known variable star
06:35:13.38 -04:56:45.4 -- not a known variable star
06:37:16.33 +03:08:55.4 -- not a known variable star
06:37:27.75 +03:09:08.7 -- a known variable star
06:37:32.00 +01:46:25.8 -- a known variable star
06:37:41.06 -03:18:49.6 -- not a known variable star
06:37:46.58 +01:47:14.8 -- not a known variable star
06:38:19.80 +02:06:04.5 -- a known variable star
06:39:07.96 +00:42:22.1 -- not a known variable star
06:40:00.34 -01:07:11.8 -- not a known variable star
06:40:30.57 -01:04:42.8 -- a known variable star
06:41:26.95 -01:17:39.5 -- not a known variable star
06:41:48.67 +01:02:03.6 -- not a known variable star
06:41:59.31 -01:11:07.3 -- a known variable star
06:42:18.78 +02:11:13.2 -- a known variable star
06:42:20.84 +02:27:50.2 -- not a known variable star
06:42:42.37 -01:42:36.7 -- not a known variable star
06:42:42.58 +03:10:33.7 -- not a known variable star
06:43:22.55 +02:17:18.7 -- a known variable star
06:43:22.75 +01:54:53.9 -- not a known variable star
06:43:50.99 +01:35:56.1 -- not a known variable star
06:43:53.97 +01:01:53.6 -- a known variable star
06:44:06.85 -00:12:06.2 -- not a known variable star
06:44:07.48 +03:13:06.7 -- not a known variable star
06:44:25.06 +01:59:02.4 -- not a known variable star
06:44:36.57 +01:45:26.7 -- not a known variable star
06:44:36.82 +00:59:54.2 -- not a known variable star
06:44:49.09 +01:46:41.0 -- not a known variable star
06:44:50.93 +01:05:44.2 -- not a known variable star
06:44:56.96 +01:18:44.4 -- not a known variable star
06:45:04.68 +02:16:56.8 -- not a known variable star
06:45:26.37 -00:11:50.4 -- not a known variable star
06:45:33.85 -00:26:17.9 -- a known variable star
06:45:39.00 +00:19:46.3 -- a known variable star
06:45:39.11 +02:45:21.6 -- a known variable star
06:45:54.21 -00:09:38.1 -- not a known variable star
06:45:55.43 +01:52:11.9 -- not a known variable star
06:45:59.16 +01:25:34.3 -- not a known variable star
06:46:09.14 +02:40:03.6 -- a known variable star
06:46:17.59 +02:25:32.7 -- a known variable star
06:46:19.51 -01:57:15.3 -- not a known variable star
06:46:22.32 +01:50:05.6 -- a known variable star
06:46:25.15 +01:49:06.0 -- not a known variable star
06:46:26.73 +00:59:01.5 -- not a known variable star
06:46:31.40 +01:08:37.5 -- not a known variable star
06:46:32.69 -01:51:14.0 -- not a known variable star
06:46:49.53 +01:25:39.2 -- not a known variable star
06:46:50.95 +01:18:08.0 -- a known variable star
06:47:02.72 +03:07:55.0 -- not a known variable star
06:47:07.64 +01:46:45.3 -- not a known variable star
06:47:10.48 +02:54:02.2 -- not a known variable star
06:47:16.50 +00:24:40.5 -- not a known variable star
06:47:18.55 +02:46:09.0 -- not a known variable star
06:47:57.05 +02:21:35.4 -- not a known variable star
06:47:59.75 -01:20:55.3 -- not a known variable star
06:48:10.05 -01:11:54.0 -- a known variable star
06:48:15.68 +01:46:15.9 -- not a known variable star
06:48:20.06 +02:20:54.5 -- not a known variable star
06:48:21.58 +01:48:27.9 -- not a known variable star
06:48:30.76 +00:57:44.2 -- not a known variable star
06:48:35.75 -00:00:05.1 -- not a known variable star
06:48:50.65 -00:08:32.1 -- not a known variable star
06:48:51.45 +02:00:14.8 -- a known variable star
06:48:57.15 -03:30:59.7 -- not a known variable star
06:48:57.56 +02:22:03.5 -- not a known variable star
06:49:07.36 -01:40:18.0 -- not a known variable star
06:49:09.02 -01:39:04.2 -- not a known variable star
06:49:11.62 +02:03:30.1 -- a known variable star
06:49:21.58 +01:13:44.4 -- not a known variable star
06:49:27.90 -03:07:23.4 -- not a known variable star
06:49:31.20 +01:58:00.6 -- not a known variable star
06:49:31.33 +02:02:03.4 -- not a known variable star
06:49:32.34 +01:56:36.0 -- not a known variable star
06:49:40.20 -01:56:05.1 -- not a known variable star
06:49:46.20 -00:13:26.0 -- not a known variable star
06:49:54.82 +02:12:16.6 -- not a known variable star
06:49:56.16 -02:17:04.6 -- not a known variable star
06:50:17.33 +02:23:27.3 -- not a known variable star
06:50:41.60 -00:31:45.7 -- not a known variable star
06:50:45.69 -01:50:53.0 -- not a known variable star
06:50:54.72 -00:02:41.4 -- not a known variable star
06:50:59.68 +00:13:38.4 -- not a known variable star
06:51:42.83 -01:56:08.2 -- not a known variable star
06:51:47.51 +02:22:37.7 -- not a known variable star
06:52:02.80 +01:24:02.6 -- not a known variable star
06:52:13.49 -00:32:56.1 -- not a known variable star
06:52:17.87 -03:21:57.5 -- not a known variable star
06:52:18.93 +03:03:40.2 -- not a known variable star
06:52:45.77 +01:05:34.7 -- not a known variable star
06:52:49.53 +03:05:07.6 -- a known variable star
06:52:54.99 -02:58:59.1 -- not a known variable star
06:52:56.47 -02:22:53.3 -- not a known variable star
06:53:35.87 +00:59:54.2 -- not a known variable star
06:53:36.83 -02:31:46.9 -- a known variable star
06:53:39.85 +01:30:57.2 -- not a known variable star
06:53:43.69 -01:58:44.8 -- not a known variable star
06:53:47.99 +00:29:47.2 -- a known variable star
06:53:50.91 -00:03:51.8 -- not a known variable star
06:54:02.36 -01:31:55.2 -- not a known variable star
06:54:03.48 +02:06:09.3 -- not a known variable star
06:54:09.37 +01:41:21.1 -- not a known variable star
06:54:26.46 +02:55:32.2 -- not a known variable star
06:54:37.42 +02:24:26.8 -- not a known variable star
06:54:39.28 +00:12:14.0 -- not a known variable star
06:54:39.55 +02:38:00.0 -- not a known variable star
06:54:40.05 +01:28:17.8 -- a known variable star
06:54:41.21 -02:07:03.7 -- a known variable star
06:55:03.35 -01:02:51.2 -- not a known variable star
06:55:11.97 +00:56:23.8 -- not a known variable star
06:55:16.01 +01:54:57.3 -- not a known variable star
06:55:16.06 +00:20:58.4 -- not a known variable star
06:55:19.17 +01:47:08.3 -- not a known variable star
06:55:20.64 +02:36:44.0 -- a known variable star
06:55:29.83 -00:58:39.6 -- not a known variable star
06:55:37.79 +02:46:12.4 -- a known variable star
06:55:38.36 +01:31:47.4 -- not a known variable star
06:55:50.82 -02:12:27.9 -- not a known variable star
06:55:54.52 +02:54:12.4 -- not a known variable star
06:55:56.43 +02:39:55.9 -- a known variable star
06:56:11.85 -01:22:24.0 -- not a known variable star
06:56:17.57 +01:28:36.3 -- a known variable star
06:56:20.94 -02:49:04.9 -- a known variable star
06:56:25.48 +00:50:44.7 -- not a known variable star
06:56:27.67 -01:27:43.2 -- not a known variable star
06:56:30.39 -01:05:52.3 -- not a known variable star
06:56:35.73 -03:00:19.8 -- not a known variable star
06:56:38.14 +00:32:04.1 -- not a known variable star
06:56:49.13 +00:46:32.2 -- not a known variable star
06:56:54.24 +00:54:12.9 -- not a known variable star
06:57:12.94 -00:34:47.9 -- not a known variable star
06:57:42.75 +01:19:13.5 -- a known variable star
06:57:47.78 -01:31:07.2 -- a known variable star
06:57:55.61 -00:57:57.2 -- a known variable star
06:58:03.77 -00:47:09.0 -- not a known variable star
06:58:04.84 +00:51:02.8 -- not a known variable star
06:58:12.09 +01:19:08.9 -- not a known variable star
06:58:19.57 -01:55:22.2 -- not a known variable star
06:58:19.95 +02:48:59.0 -- not a known variable star
06:58:20.22 -00:33:16.9 -- not a known variable star
06:58:26.17 -00:35:49.9 -- not a known variable star
06:58:30.49 +00:42:34.4 -- not a known variable star
06:58:34.29 -01:38:14.7 -- not a known variable star
06:58:36.41 -00:17:14.6 -- not a known variable star
06:58:39.27 -01:55:22.2 -- not a known variable star
06:58:48.13 -00:36:48.6 -- not a known variable star
06:58:57.13 -03:00:42.3 -- not a known variable star
06:59:00.28 -01:14:43.0 -- a known variable star
06:59:00.81 +00:17:55.9 -- not a known variable star
06:59:01.10 -02:36:01.4 -- not a known variable star
06:59:25.54 +01:32:51.5 -- not a known variable star
06:59:35.85 -00:50:16.2 -- a known variable star
06:59:40.61 -00:39:47.8 -- not a known variable star
06:59:42.47 +00:17:26.2 -- a known variable star
06:59:44.36 -01:15:43.1 -- not a known variable star
06:59:46.73 -02:22:11.0 -- not a known variable star
06:59:56.94 +02:16:59.9 -- not a known variable star
07:00:01.82 +00:36:59.6 -- not a known variable star
07:00:16.18 +01:37:06.9 -- not a known variable star
07:00:17.01 +01:41:49.3 -- not a known variable star
07:00:20.28 +01:48:26.0 -- not a known variable star
07:00:26.60 -00:13:24.1 -- not a known variable star
07:00:29.10 +02:41:10.2 -- not a known variable star
07:00:33.00 -02:10:37.1 -- not a known variable star
07:00:38.82 -01:30:48.4 -- not a known variable star
07:00:52.11 +00:11:59.2 -- not a known variable star
07:01:02.14 +01:28:24.6 -- not a known variable star
07:01:04.49 +00:15:12.0 -- a known variable star
07:01:11.28 -00:44:18.2 -- not a known variable star
07:01:14.63 +00:57:27.1 -- not a known variable star
07:01:18.64 -03:25:50.7 -- not a known variable star
07:01:19.21 -03:06:43.4 -- not a known variable star
07:01:28.73 -01:08:32.7 -- a known variable star
07:01:30.56 +00:16:28.3 -- a known variable star
07:01:31.08 -00:10:46.0 -- not a known variable star
07:01:47.31 -00:22:58.6 -- a known variable star
07:01:58.24 -02:16:30.3 -- not a known variable star
07:02:02.52 -02:08:44.8 -- not a known variable star
07:02:13.85 -00:12:25.2 -- not a known variable star
07:02:13.97 -01:26:47.7 -- not a known variable star
07:02:14.33 -00:35:02.5 -- not a known variable star
07:02:18.17 +01:30:39.3 -- a known variable star
07:02:18.29 -02:01:26.0 -- not a known variable star
07:02:21.27 -03:20:49.8 -- not a known variable star
07:02:25.57 -01:07:14.1 -- a known variable star
07:02:37.68 -01:54:04.8 -- not a known variable star
07:02:38.04 -00:50:21.9 -- a known variable star
07:02:39.71 +01:10:07.4 -- a known variable star
07:02:44.61 +02:16:17.0 -- not a known variable star
07:02:49.63 -03:11:35.6 -- a known variable star
07:02:55.62 +02:43:38.3 -- not a known variable star
07:02:55.80 -02:02:38.7 -- not a known variable star
07:03:10.94 +01:19:42.5 -- not a known variable star
07:03:12.32 +01:32:44.2 -- a known variable star
07:03:36.97 +02:37:09.5 -- a known variable star
07:03:37.07 -00:12:39.1 -- not a known variable star
07:03:41.13 -02:10:56.7 -- not a known variable star
07:03:46.12 -02:09:36.6 -- not a known variable star
07:03:53.68 +01:24:54.1 -- not a known variable star
07:03:54.33 -00:57:01.3 -- not a known variable star
07:04:11.72 -01:14:21.1 -- a known variable star
07:04:16.83 -03:01:34.4 -- not a known variable star
07:04:18.50 -03:01:59.9 -- not a known variable star
07:04:20.04 +00:50:07.5 -- not a known variable star
07:04:22.61 +00:59:50.4 -- not a known variable star
07:04:33.37 +01:07:10.0 -- a known variable star
07:04:36.28 +02:03:16.2 -- not a known variable star
07:04:40.26 -01:02:14.9 -- not a known variable star
07:04:46.70 +02:30:40.5 -- not a known variable star
07:04:51.44 -02:16:54.6 -- a known variable star
07:04:51.69 -02:12:04.6 -- not a known variable star
07:04:51.78 -00:22:11.6 -- not a known variable star
07:04:54.75 +00:11:37.4 -- not a known variable star
07:05:01.79 +01:30:35.3 -- not a known variable star
07:05:14.72 +00:02:12.7 -- not a known variable star
07:05:15.75 +00:02:26.7 -- not a known variable star
07:05:18.14 -01:22:58.9 -- a known variable star
07:05:20.65 +02:45:55.3 -- not a known variable star
07:05:25.69 -00:15:24.7 -- not a known variable star
07:05:26.28 +01:29:35.0 -- a known variable star
07:05:28.89 -02:00:10.0 -- a known variable star
07:05:33.88 +02:07:16.9 -- not a known variable star
07:05:37.67 +02:21:34.8 -- not a known variable star
07:05:38.92 -00:02:18.2 -- not a known variable star
07:05:41.37 +00:53:11.5 -- a known variable star
07:05:41.63 +02:40:14.3 -- a known variable star
07:05:44.55 +00:49:31.5 -- a known variable star
07:05:47.91 +00:29:01.2 -- not a known variable star
07:05:49.37 +02:34:30.1 -- not a known variable star
07:05:57.89 +02:49:16.7 -- not a known variable star
07:06:07.44 -01:56:14.6 -- not a known variable star
07:06:11.37 +00:35:33.6 -- not a known variable star
07:06:20.25 +02:30:43.9 -- not a known variable star
07:06:28.80 -02:56:50.2 -- not a known variable star
07:06:29.13 +02:03:03.8 -- not a known variable star
07:06:31.79 +02:11:35.5 -- a known variable star
07:06:45.79 -01:30:48.7 -- a known variable star
07:06:47.77 -02:29:52.1 -- not a known variable star
07:06:54.27 +02:10:48.7 -- a known variable star
07:06:55.30 +00:27:40.6 -- a known variable star
07:07:03.77 -02:21:49.1 -- not a known variable star
07:07:06.88 +01:52:33.3 -- not a known variable star
07:07:06.99 +01:39:59.7 -- not a known variable star
07:07:15.29 -02:45:48.6 -- not a known variable star
07:07:24.37 -01:20:26.7 -- a known variable star
07:07:26.07 -01:50:44.5 -- not a known variable star
07:07:26.39 +01:04:08.9 -- a known variable star
07:08:04.63 -01:43:42.0 -- not a known variable star
07:08:17.08 -00:08:18.5 -- a known variable star
07:08:21.83 -02:47:11.8 -- a known variable star
07:08:21.93 +01:09:06.7 -- not a known variable star
07:08:24.38 +01:25:13.8 -- not a known variable star
07:08:25.07 +02:46:18.0 -- not a known variable star
07:08:30.79 +01:18:17.1 -- not a known variable star
07:08:43.48 +01:22:16.7 -- not a known variable star
07:08:45.38 +00:41:47.6 -- a known variable star
07:08:46.25 -02:21:30.9 -- not a known variable star
07:08:49.41 -00:04:35.3 -- a known variable star
07:08:58.14 -02:02:45.9 -- not a known variable star
07:09:05.12 +01:56:10.4 -- not a known variable star
07:09:13.73 -02:21:30.2 -- a known variable star
07:09:18.35 +00:20:29.3 -- not a known variable star
07:09:20.73 +02:38:44.8 -- not a known variable star
07:09:21.74 +01:07:27.4 -- a known variable star
07:09:27.00 -01:59:51.6 -- a known variable star
07:09:29.63 -02:28:31.9 -- not a known variable star
07:09:36.62 +01:42:30.9 -- not a known variable star
07:09:37.95 -00:01:19.0 -- a known variable star
07:09:56.82 -00:13:56.2 -- not a known variable star
07:10:07.72 -02:09:54.0 -- a known variable star
07:10:09.29 +00:56:13.2 -- not a known variable star
07:10:10.11 -00:03:48.8 -- not a known variable star
07:10:12.72 +01:37:53.5 -- a known variable star
07:10:14.51 +02:07:07.6 -- not a known variable star
07:10:27.43 -01:29:57.0 -- not a known variable star
07:10:27.68 -00:31:02.8 -- not a known variable star
07:10:31.35 -00:55:58.4 -- a known variable star
07:10:36.57 +00:49:12.4 -- not a known variable star
07:10:39.38 +00:54:03.6 -- a known variable star
07:10:42.79 -01:49:36.7 -- not a known variable star
07:10:51.48 +00:26:29.0 -- a known variable star
07:10:55.26 -00:54:17.3 -- not a known variable star
07:10:59.27 -02:27:10.6 -- a known variable star
07:11:04.92 +01:22:09.1 -- not a known variable star
07:11:17.16 -01:29:12.8 -- a known variable star
07:11:19.12 -00:54:11.8 -- not a known variable star
07:11:19.89 -02:24:45.1 -- not a known variable star
07:11:20.26 +01:36:57.3 -- not a known variable star
07:11:21.13 +00:51:01.2 -- not a known variable star
07:11:22.57 -01:09:07.0 -- a known variable star
07:11:29.19 +00:13:44.9 -- not a known variable star
07:11:30.41 +00:31:16.9 -- not a known variable star
07:11:30.95 +02:07:35.0 -- not a known variable star
07:11:32.72 -01:56:46.4 -- a known variable star
07:11:38.36 +01:05:43.8 -- not a known variable star
07:11:40.10 -00:09:33.5 -- not a known variable star
07:11:46.26 +01:10:53.3 -- not a known variable star
07:11:50.22 +01:54:46.4 -- not a known variable star
07:11:50.34 +01:30:56.8 -- not a known variable star
07:11:51.77 +01:45:14.1 -- not a known variable star
07:12:25.57 +01:03:06.8 -- not a known variable star
07:12:50.13 +01:20:16.7 -- not a known variable star
07:12:55.05 -01:57:59.6 -- not a known variable star
07:12:56.34 +02:36:38.9 -- not a known variable star
07:12:57.03 +00:52:08.2 -- a known variable star
07:13:00.83 -00:32:50.3 -- not a known variable star
07:13:12.67 +01:29:20.3 -- a known variable star
07:13:12.96 +01:58:09.4 -- not a known variable star
07:13:26.15 -00:17:23.7 -- a known variable star
07:13:34.41 +01:59:23.2 -- not a known variable star
07:13:40.87 -01:01:27.1 -- not a known variable star
07:13:48.52 +02:30:38.5 -- not a known variable star
07:13:50.86 +01:53:48.9 -- not a known variable star
07:13:59.16 -01:53:58.4 -- not a known variable star
07:13:59.68 -00:06:57.6 -- not a known variable star
07:14:00.58 -01:15:32.7 -- not a known variable star
07:14:15.01 +02:36:26.0 -- not a known variable star
07:14:24.74 +01:01:59.9 -- not a known variable star
07:14:29.98 +01:49:07.0 -- not a known variable star
07:14:33.98 +01:07:26.5 -- not a known variable star
07:14:36.80 -01:22:24.8 -- not a known variable star
07:14:45.41 -01:22:50.9 -- not a known variable star
07:14:48.01 +01:49:34.7 -- not a known variable star
07:14:59.24 -01:45:23.7 -- not a known variable star
07:15:02.37 -01:57:47.6 -- not a known variable star
07:15:07.58 +02:26:31.9 -- not a known variable star
07:15:08.76 +00:57:28.1 -- a known variable star
07:15:31.52 +02:29:20.0 -- not a known variable star
07:15:33.21 -01:08:35.0 -- not a known variable star
07:15:39.68 -00:49:28.5 -- not a known variable star
07:15:46.04 -02:39:24.6 -- not a known variable star
07:15:57.43 +02:41:29.0 -- a known variable star
07:16:03.24 -00:40:40.0 -- not a known variable star
07:16:05.29 +01:51:25.9 -- not a known variable star
07:16:12.26 -00:07:08.2 -- not a known variable star
07:16:21.46 +00:55:10.1 -- not a known variable star
07:16:40.64 -01:23:41.7 -- not a known variable star
07:16:42.04 +02:29:03.9 -- not a known variable star
07:16:43.51 +01:09:10.0 -- not a known variable star
07:17:28.21 -01:37:00.1 -- a known variable star
07:17:31.31 +01:05:38.1 -- a known variable star
07:17:33.59 -01:43:04.5 -- not a known variable star
07:17:34.67 +00:34:44.7 -- not a known variable star
07:17:57.96 +00:42:48.4 -- not a known variable star
07:18:00.93 -01:12:31.8 -- not a known variable star
07:18:11.59 +02:33:20.1 -- a known variable star
07:18:12.11 -02:02:25.6 -- not a known variable star
07:18:21.30 -00:48:11.5 -- not a known variable star
07:18:23.32 +01:03:40.2 -- a known variable star
07:18:26.98 +00:26:42.9 -- not a known variable star
07:18:29.97 -00:11:37.0 -- not a known variable star
07:18:41.69 +01:11:02.7 -- a known variable star
07:18:45.41 +02:22:33.7 -- not a known variable star
07:18:48.77 -01:43:45.9 -- not a known variable star
07:18:50.08 -00:32:54.1 -- not a known variable star
07:18:57.19 -00:43:48.7 -- not a known variable star
07:18:59.78 -00:08:13.5 -- not a known variable star
07:19:25.60 -02:06:13.4 -- not a known variable star
07:19:46.39 +00:48:05.1 -- not a known variable star
07:19:47.36 -00:02:48.7 -- not a known variable star
07:19:50.64 +00:15:40.1 -- not a known variable star
07:20:15.60 -02:00:46.4 -- not a known variable star
07:20:16.54 +01:20:10.0 -- a known variable star
07:20:34.20 -00:45:30.2 -- not a known variable star
07:20:50.44 -00:51:22.6 -- a known variable star
07:21:14.52 -01:19:48.9 -- not a known variable star
07:21:32.43 -00:16:17.2 -- a known variable star
07:21:35.99 +00:47:41.0 -- not a known variable star
07:21:37.21 +00:28:48.2 -- not a known variable star
07:21:50.20 +00:09:22.6 -- not a known variable star
07:22:20.08 -01:09:42.1 -- a known variable star
Found 287 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
381 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 381 (excluding asteroids and hot pixels, 287 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)2461146.61270135 -observatory V36
00:07:52.59 -01:59:50.4 Mercury (0.0mag)
03:09:11.67 +17:54:00.5 Venus (-3.9mag)
00:18:09.62 +00:54:00.2 Mars (1.2mag)
07:12:40.92 +22:46:09.0 Jupiter (-2.1mag)
00:29:13.88 +00:49:17.7 Saturn (0.9mag)
03:47:43.24 +19:47:33.2 Uranus (5.8mag)
00:10:51.30 -00:15:16.7 Neptune (7.8mag)
20:33:45.56 -22:52:36.2 Pluto (14.5mag)
00:19:38.99 +04:32:51.4 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 361 Apr 15 22:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461146.61270135:
07:12:42.12 +22:46:09.0 Io (5.8mag)
07:12:46.26 +22:46:00.2 Europa (5.9mag)
07:12:57.96 +22:45:29.6 Ganymede (5.4mag)
07:13:16.29 +22:44:56.7 Callisto (6.6mag)
07:16:00.86 +22:33:43.4 Himalia (15.3mag)
07:12:39.28 +22:46:10.4 Thebe (16.2mag)
07:16:12.39 +23:03:55.6 Elara (17.3mag)
07:11:34.26 +23:26:05.8 Pasiphae (17.4mag)
07:21:00.47 +22:44:11.0 Carme (18.5mag)
00:29:14.43 +00:49:43.9 Titan (8.8mag)
00:29:12.33 +00:49:21.9 Rhea (10.1mag)
00:28:53.70 +00:49:26.0 Iapetus (11.5mag)
00:29:21.79 +00:49:37.8 Hyperion (14.8mag)
00:30:50.68 +00:58:05.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 15 22:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.61270135:
15:38:59.46 -16:18:56.1 JWST
13:14:47.83 +54:12:26.1 Chandra
07:51:19.70 -33:45:37.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 15 22:35 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.61270135 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:02.99 -28:47:07.5 13.9mag P/2010 H2 (Vales)
05:06:48.91 -69:39:23.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:28.21 +31:26:17.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:25.51 +10:33:39.7 17.6mag C/2021 G2 (ATLAS)
23:10:15.24 +29:13:59.9 17.1mag C/2022 E2 (ATLAS)
04:29:22.03 +26:02:29.6 16.0mag C/2022 N2 (PANSTARRS)
09:03:26.66 +32:01:06.3 16.2mag C/2022 QE78 (ATLAS)
08:31:05.42 -00:08:28.2 17.3mag C/2022 R6 (PANSTARRS)
18:53:42.31 +18:32:30.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:38.33 -11:31:11.8 17.5mag P/2023 B1 (PANSTARRS)
09:07:35.00 -11:51:54.4 17.6mag C/2023 F3 (ATLAS)
21:54:19.69 +62:54:46.2 17.5mag C/2023 H5 (Lemmon)
19:19:06.18 -03:44:03.5 14.1mag C/2023 R1 (PANSTARRS)
21:32:18.97 +85:55:36.8 17.8mag C/2023 X2 (Lemmon)
06:17:56.95 +63:30:45.3 17.2mag C/2024 A1 (ATLAS)
05:13:31.07 +18:20:45.9 11.1mag C/2024 E1 (Wierzchos)
16:19:12.29 +06:24:32.1 17.4mag C/2024 G6 (ATLAS)
20:20:50.61 +15:18:17.5 14.6mag C/2024 J3 (ATLAS)
03:26:28.13 -22:22:06.2 16.3mag C/2024 T5 (ATLAS)
05:16:48.45 +45:15:47.3 17.7mag C/2025 J1 (Borisov)
13:38:22.16 +45:33:52.2 15.2mag C/2025 L1 (ATLAS)
03:25:27.11 -26:13:45.6 17.8mag C/2025 Q3 (ATLAS)
23:44:23.50 +18:34:31.7 8.5mag C/2025 R3 (PANSTARRS)
12:54:04.21 +03:01:10.8 17.4mag C/2025 Y1 (ATLAS)
03:28:51.88 +02:36:28.5 13.3mag C/2026 A1 (MAPS)
23:59:53.95 +37:14:25.2 14.6mag C/2026 B2 (Sun-Gao)
18:43:09.25 -09:42:46.8 11.8mag 10P/Tempel
15:00:09.43 +03:11:51.6 14.0mag 24P/Schaumasse
11:02:46.36 -01:31:21.1 15.7mag 29P/Schwassmann-Wachmann
18:00:59.79 -09:36:21.2 17.9mag 40P/Vaisala
10:37:33.62 -04:05:23.5 16.9mag 43P/Wolf-Harrington
01:48:50.82 +17:30:24.9 17.2mag 47P/Ashbrook-Jackson
07:10:58.31 +36:59:20.0 17.0mag 63P/Wild
23:29:12.02 -11:26:14.2 15.7mag 65P/Gunn
04:03:32.91 +21:17:38.7 15.9mag 76P/West-Kohoutek-Ikemura
01:05:49.36 +08:15:03.2 14.3mag 78P/Gehrels
23:03:20.62 -09:21:28.1 14.6mag 88P/Howell
02:10:43.03 +20:40:21.3 15.1mag 93P/Lovas
04:55:00.87 +32:17:38.4 16.2mag 123P/West-Hartley
08:28:29.71 +38:18:33.9 16.2mag 124P/Mrkos
02:33:23.33 +14:22:57.5 16.4mag 128P/Shoemaker-Holt
02:47:45.43 +14:30:25.4 17.5mag 131P/Mueller
01:26:45.25 +13:16:40.0 10.6mag 141P/Machholz
01:35:40.10 +04:54:58.1 10.6mag 141P-A/Machholz
00:20:54.48 +00:49:16.3 12.8mag 141P-D/Machholz
02:06:00.41 +06:40:30.8 17.8mag 141P-I/Machholz
01:02:41.46 -01:28:08.9 15.1mag 162P/SidingSpring
14:51:14.12 -00:03:22.5 17.6mag 210P/Christensen
21:39:10.32 -11:25:16.8 17.6mag 218P/LINEAR
17:16:35.85 -13:55:10.5 16.1mag 235P/LINEAR
05:34:43.49 +34:42:27.8 16.8mag 240P/NEAT
07:38:32.93 -05:09:17.6 17.7mag 242P/Spahr
22:17:11.32 -20:57:00.4 17.9mag 260P/McNaught
01:58:25.07 +20:29:20.9 18.0mag 295P/LINEAR
15:42:36.20 +06:59:52.7 17.5mag 391P/Kowalski
07:34:14.33 +21:21:59.3 17.7mag 450P/LONEOS
05:36:02.06 +45:01:34.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 15 22:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
-rw-r--r-- 1 apache apache 5.8K Apr 15 22:35 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 15 22:35 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:52:32.558 +54:28:28.21 AT 2026iyo 2026-04-07.50 19.8736
12:10:51.131 -15:24:05.80 AT 2026iyn 2026-04-07.49 19.8
10:03:32.464 +00:47:38.92 AT 2026iym 2026-04-09.07 21.7842
09:57:46.577 +02:32:54.17 AT 2026iyl 2026-04-09.07 21.1159
12:09:21.288 -14:20:40.69 AT 2026iyk 2026-02-24.42 19.0617
11:32:15.323 +26:34:23.97 AT 2026iyi 2026-04-07.27 20.0038
08:41:36.643 +41:14:51.53 AT 2026iyh 2026-03-18.28 20.5874
11:10:47.748 -02:27:00.61 AT 2026iyg 2026-04-07.26 20.12
11:41:25.329 -11:32:16.55 AT 2026iyf 2026-04-07.25 20.8489
09:58:35.594 -17:44:37.57 AT 2026iye 2026-04-08.19 19.4848
07:48:08.582 +43:35:35.35 AT 2026iyd 2026-04-05.16 19.8382
11:13:43.729 +21:50:31.84 AT 2026iyc 2026-04-05.18 20.0005
08:02:45.458 +40:40:22.73 AT 2026iyb 2026-03-26.18 20.4831
13:05:52.496 +64:22:32.75 AT 2026iya 2026-03-08.94 19.29
05:15:26.423 -02:54:24.54 AT 2026ixz 2026-04-08.14 19.1905
14:04:24.118 +43:40:15.80 AT 2026ixt 2026-04-08.93 19.74
13:12:41.279 +38:05:24.08 AT 2026ixs 2026-04-08.93 20.18
13:21:56.843 -04:01:33.33 AT 2026ixr 2026-04-08.90 19.48
12:04:52.343 +69:44:57.80 AT 2026ixq 2026-04-08.89 19.03
21:31:46.671 +04:33:36.35 AT 2026ixp 2026-04-08.51 19.1697
-rw-r--r-- 1 apache apache 30K Apr 15 22:35 tns_transients_list.txt
