This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o
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
target,2461148.6171,13.78,0.05,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
target 20260418.1171 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
Gaia DR3 3119756014938079616,2461148.6171,13.72,0.05,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
Gaia DR3 3119756014938079616 20260418.1171 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 3112569950538238464,2461148.6171,13.70,0.05,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 3112569950538238464 20260418.1171 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 J104.0605-03.8344,2461148.6171,13.67,0.05,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 J104.0605-03.8344 20260418.1171 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,2461148.6171,13.56,0.05,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 20260418.1171 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3978+03.1340,2461148.6171,13.62,0.05,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 J101.3978+03.1340 20260418.1171 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 3109065394664787200,2461148.6171,13.73,0.05,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 3109065394664787200 20260418.1171 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,2461148.6171,13.50,0.05,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
target 20260418.1171 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
target,2461148.6171,13.62,0.05,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 20260418.1171 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 J105.7164-04.9963,2461148.6171,13.55,0.05,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 J105.7164-04.9963 20260418.1171 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 3113168664678149376,2461148.6171,13.45,0.05,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 3113168664678149376 20260418.1171 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
target,2461148.6171,13.49,0.05,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 20260418.1171 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,2461148.6171,13.49,0.05,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 20260418.1171 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,2461148.6171,13.45,0.05,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
target 20260418.1171 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 J105.4041-04.5455,2461148.6171,13.55,0.05,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 J105.4041-04.5455 20260418.1171 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 J102.6870+01.0515,2461148.6171,13.52,0.05,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 J102.6870+01.0515 20260418.1171 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 J105.7753-05.2912,2461148.6171,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.7753-05.2912 20260418.1171 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.9221+01.1622,2461148.6171,13.30,0.05,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
ATO J099.9221+01.1622 20260418.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.33,0.05,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 20260418.1171 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
target,2461148.6171,13.34,0.05,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 20260418.1171 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,2461148.6171,13.25,0.05,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
target 20260418.1171 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 3109907586213358720,2461148.6171,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109907586213358720 20260418.1171 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.27,0.05,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 20260418.1171 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111507508770537216,2461148.6171,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111507508770537216 20260418.1171 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.24,0.05,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
target 20260418.1171 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,2461148.6171,13.20,0.05,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
target 20260418.1171 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1615-01.5148,2461148.6171,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1615-01.5148 20260418.1171 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 3109432768987249664,2461148.6171,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109432768987249664 20260418.1171 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 3112803528038358144,2461148.6171,13.24,0.05,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 3112803528038358144 20260418.1171 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 J107.8770+00.5215,2461148.6171,13.21,0.05,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 20260418.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0207+00.9747,2461148.6171,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0207+00.9747 20260418.1171 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.22,0.05,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
target 20260418.1171 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107406673992729472,2461148.6171,13.06,0.05,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 3107406673992729472 20260418.1171 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110181055368994560,2461148.6171,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110181055368994560 20260418.1171 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
target,2461148.6171,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461148.6171,12.96,0.05,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
target 20260418.1171 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.12,0.05,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
target 20260418.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120464375303293312,2461148.6171,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120464375303293312 20260418.1171 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9070-06.5989,2461148.6171,12.97,0.05,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 J107.9070-06.5989 20260418.1171 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
Gaia DR3 3113068166743350016,2461148.6171,12.97,0.05,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 3113068166743350016 20260418.1171 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 J109.8492-02.7067,2461148.6171,12.99,0.05,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 J109.8492-02.7067 20260418.1171 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5396-00.9195,2461148.6171,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5396-00.9195 20260418.1171 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.1701-03.5709,2461148.6171,12.98,0.05,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
ATO J110.1701-03.5709 20260418.1171 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125849023043907328,2461148.6171,13.07,0.05,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 3125849023043907328 20260418.1171 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 3116003450473542784,2461148.6171,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3116003450473542784 20260418.1171 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J109.9050-02.3273,2461148.6171,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.9050-02.3273 20260418.1171 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
ATO J110.3547-03.5841,2461148.6171,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.3547-03.5841 20260418.1171 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107197805444320128,2461148.6171,12.77,0.05,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 3107197805444320128 20260418.1171 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.6431-01.9595,2461148.6171,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.6431-01.9595 20260418.1171 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114569137555198464,2461148.6171,12.80,0.05,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 3114569137555198464 20260418.1171 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.2010-06.2724,2461148.6171,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.2010-06.2724 20260418.1171 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059427667355169920,2461148.6171,12.96,0.05,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 3059427667355169920 20260418.1171 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3502-00.8380,2461148.6171,12.79,0.05,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
ATO J104.3502-00.8380 20260418.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109841924755441024,2461148.6171,12.77,0.05,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 3109841924755441024 20260418.1171 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3057972115815283328,2461148.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3057972115815283328 20260418.1171 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7707-03.1723,2461148.6171,12.71,0.05,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 J106.7707-03.1723 20260418.1171 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,12.54,0.05,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
target 20260418.1171 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115633327372214656,2461148.6171,12.66,0.05,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 3115633327372214656 20260418.1171 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
ATO J108.5157-01.0853,2461148.6171,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.5157-01.0853 20260418.1171 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
ATO J107.5597-00.8073,2461148.6171,12.63,0.05,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 J107.5597-00.8073 20260418.1171 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
ATO J102.3654+02.4200,2461148.6171,12.58,0.05,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 J102.3654+02.4200 20260418.1171 12.58CV 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,2461148.6171,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1998+01.9832,2461148.6171,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1998+01.9832 20260418.1171 12.51CV 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 J107.0950-01.3341,2461148.6171,12.41,0.05,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
ATO J107.0950-01.3341 20260418.1171 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 J106.3136-06.0776,2461148.6171,12.34,0.05,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
ATO J106.3136-06.0776 20260418.1171 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3269-02.4900,2461148.6171,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3269-02.4900 20260418.1171 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112143821063478656,2461148.6171,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112143821063478656 20260418.1171 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111293898573338368,2461148.6171,12.21,0.05,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 3111293898573338368 20260418.1171 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,2461148.6171,12.10,0.05,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
target 20260418.1171 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
Gaia DR3 3108464610338813696,2461148.6171,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108464610338813696 20260418.1171 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112151242766551808,2461148.6171,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112151242766551808 20260418.1171 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112361520064709376,2461148.6171,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112361520064709376 20260418.1171 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12569794,2461148.6171,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12569794 20260418.1171 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822923819222400,2461148.6171,9.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822923819222400 20260418.1171 9.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.0773+01.7811,2461148.6171,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.0773+01.7811 20260418.1171 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1631+01.7787,2461148.6171,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260418.1171 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461148.6171,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260418.1171 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113311193174967552,2461148.6171,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113311193174967552 20260418.1171 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112051973180962048,2461148.6171,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112051973180962048 20260418.1171 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115211321064418944,2461148.6171,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115211321064418944 20260418.1171 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112803768556485248,2461148.6171,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112803768556485248 20260418.1171 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119280785395344512,2461148.6171,12.22,0.05,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
Gaia DR3 3119280785395344512 20260418.1171 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.2900+02.4888,2461148.6171,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.2900+02.4888 20260418.1171 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3035-03.3194,2461148.6171,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3035-03.3194 20260418.1171 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100858296278549504,2461148.6171,12.41,0.05,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 3100858296278549504 20260418.1171 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
ASASSN-V J064143.42-010627.5,2461148.6171,12.60,0.05,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
ASASSN-V J064143.42-010627.5 20260418.1171 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
ATO J100.6477-03.4721,2461148.6171,12.64,0.05,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
ATO J100.6477-03.4721 20260418.1171 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7920-02.0410,2461148.6171,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7920-02.0410 20260418.1171 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.7792+02.6881,2461148.6171,12.52,0.05,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 J108.7792+02.6881 20260418.1171 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 3110006336102386176,2461148.6171,12.50,0.05,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
Gaia DR3 3110006336102386176 20260418.1171 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
Gaia DR3 3113103071939549184,2461148.6171,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113103071939549184 20260418.1171 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0122+02.1631,2461148.6171,12.61,0.05,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
ATO J109.0122+02.1631 20260418.1171 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109346732203582208,2461148.6171,12.72,0.05,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 3109346732203582208 20260418.1171 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
Gaia DR3 3115718642601361280,2461148.6171,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115718642601361280 20260418.1171 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8701-01.1937,2461148.6171,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.8701-01.1937 20260418.1171 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107474882374152960,2461148.6171,12.65,0.05,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
Gaia DR3 3107474882374152960 20260418.1171 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109532137349277568,2461148.6171,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109532137349277568 20260418.1171 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461148.6171,12.56,0.05,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
ATO J100.9580+01.5948 20260418.1171 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
Gaia DR3 3109436308041776640,2461148.6171,12.49,0.05,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 3109436308041776640 20260418.1171 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120812576892617856,2461148.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120812576892617856 20260418.1171 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127764887696264704,2461148.6171,12.63,0.05,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 3127764887696264704 20260418.1171 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
target,2461148.6171,12.66,0.05,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
target 20260418.1171 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
GDS_J0707331-032533,2461148.6171,12.68,0.05,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
GDS_J0707331-032533 20260418.1171 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2998-03.9607,2461148.6171,12.77,0.05,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 J104.2998-03.9607 20260418.1171 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461148.6171,12.64,0.05,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 3114694099624336256 20260418.1171 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461148.6171,12.68,0.05,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 J106.0676-03.0161 20260418.1171 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5494+00.3110,2461148.6171,12.71,0.05,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 J106.5494+00.3110 20260418.1171 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.1593+02.9125,2461148.6171,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.1593+02.9125 20260418.1171 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461148.6171,12.80,0.05,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 3126271617766100608 20260418.1171 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7477+00.2283,2461148.6171,12.79,0.05,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
ATO J102.7477+00.2283 20260418.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071155.48-045255.5,2461148.6171,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071155.48-045255.5 20260418.1171 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302487915881984,2461148.6171,12.79,0.05,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 3105302487915881984 20260418.1171 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.1463-06.9005,2461148.6171,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.1463-06.9005 20260418.1171 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,12.93,0.05,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
target 20260418.1171 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.2675-03.2520,2461148.6171,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.2675-03.2520 20260418.1171 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127213516974967296,2461148.6171,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127213516974967296 20260418.1171 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107920768701471488,2461148.6171,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107920768701471488 20260418.1171 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
ATO J108.7910+00.3663,2461148.6171,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.7910+00.3663 20260418.1171 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0276-01.3052,2461148.6171,13.10,0.05,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 J103.0276-01.3052 20260418.1171 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 3103464959174981120,2461148.6171,12.97,0.05,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 3103464959174981120 20260418.1171 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
Gaia DR3 3104844811903742208,2461148.6171,12.98,0.05,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 3104844811903742208 20260418.1171 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461148.6171,13.04,0.05,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 20260418.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BEST-II lra2a_00642,2461148.6171,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BEST-II lra2a_00642 20260418.1171 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101029201615746048,2461148.6171,12.99,0.05,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 3101029201615746048 20260418.1171 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461148.6171,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102785122 20260418.1171 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102806577,2461148.6171,13.11,0.05,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
CoRoT 102806577 20260418.1171 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 3125762818759969664,2461148.6171,13.01,0.05,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 3125762818759969664 20260418.1171 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 J103.6945-01.2944,2461148.6171,13.08,0.05,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 J103.6945-01.2944 20260418.1171 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3566-03.3095,2461148.6171,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3566-03.3095 20260418.1171 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 3125637852391270784,2461148.6171,13.11,0.05,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 20260418.1171 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 3111159380198287232,2461148.6171,13.03,0.05,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 3111159380198287232 20260418.1171 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461148.6171,13.04,0.05,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 3114460526421262848 20260418.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070654.13+021046.6,2461148.6171,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070654.13+021046.6 20260418.1171 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 3125607134785759744,2461148.6171,13.04,0.05,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 3125607134785759744 20260418.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125922381086607360,2461148.6171,13.06,0.05,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 3125922381086607360 20260418.1171 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108090471452077184,2461148.6171,13.00,0.05,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 3108090471452077184 20260418.1171 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 3112672888012933248,2461148.6171,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112672888012933248 20260418.1171 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.6375-01.8671,2461148.6171,13.21,0.05,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 J101.6375-01.8671 20260418.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461148.6171,13.18,0.05,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 J101.9913-01.3476 20260418.1171 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
target,2461148.6171,13.06,0.05,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 20260418.1171 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.10,0.05,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
target 20260418.1171 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 3118957632057909376,2461148.6171,13.16,0.05,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 3118957632057909376 20260418.1171 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
[KEE2007] 2083,2461148.6171,13.30,0.05,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
[KEE2007] 2083 20260418.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108875037414575232,2461148.6171,13.12,0.05,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 3108875037414575232 20260418.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115421087268758272,2461148.6171,13.04,0.05,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 3115421087268758272 20260418.1171 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.6707-05.7846,2461148.6171,13.21,0.05,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 J101.6707-05.7846 20260418.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108798488219749888,2461148.6171,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108798488219749888 20260418.1171 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 J099.5776-03.3486,2461148.6171,13.21,0.05,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 J099.5776-03.3486 20260418.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.0643-00.0070,2461148.6171,13.33,0.05,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
ATO J101.0643-00.0070 20260418.1171 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
Gaia DR3 3127203655728648192,2461148.6171,13.12,0.05,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 3127203655728648192 20260418.1171 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.21,0.05,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 20260418.1171 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112456559100452352,2461148.6171,13.24,0.05,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 3112456559100452352 20260418.1171 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,2461148.6171,13.30,0.05,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 20260418.1171 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114638612946099072,2461148.6171,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114638612946099072 20260418.1171 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0837+00.8377,2461148.6171,13.37,0.05,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 J106.0837+00.8377 20260418.1171 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.8673+00.4997,2461148.6171,13.47,0.05,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 J098.8673+00.4997 20260418.1171 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.38,0.05,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 20260418.1171 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
ASASSN-V J063337.12+022003.1,2461148.6171,13.46,0.05,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
ASASSN-V J063337.12+022003.1 20260418.1171 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 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 J101.1511+00.9977,2461148.6171,13.31,0.05,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 J101.1511+00.9977 20260418.1171 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126180736259064064,2461148.6171,13.44,0.05,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 3126180736259064064 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.57,0.05,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
target 20260418.1171 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
ATO J103.4491-02.6658,2461148.6171,13.36,0.05,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 J103.4491-02.6658 20260418.1171 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3333-01.1994,2461148.6171,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3333-01.1994 20260418.1171 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126373180854468736,2461148.6171,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126373180854468736 20260418.1171 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119355071151771648,2461148.6171,13.34,0.05,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 3119355071151771648 20260418.1171 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 3106945708044956416,2461148.6171,13.44,0.05,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 3106945708044956416 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113353627450988288,2461148.6171,13.47,0.05,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 3113353627450988288 20260418.1171 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.51,0.05,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 20260418.1171 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1889-04.3742,2461148.6171,13.44,0.05,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 J101.1889-04.3742 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102494433997697024,2461148.6171,13.60,0.05,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 3102494433997697024 20260418.1171 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
ZTF J064842.74+020218.5,2461148.6171,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J064842.74+020218.5 20260418.1171 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 J101.5488+00.7303,2461148.6171,13.44,0.05,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 J101.5488+00.7303 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6538+02.9708,2461148.6171,13.52,0.05,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 J100.6538+02.9708 20260418.1171 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,2461148.6171,13.34,0.05,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 20260418.1171 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,2461148.6171,13.57,0.05,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
target 20260418.1171 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
Gaia DR3 3108105383578700928,2461148.6171,13.54,0.05,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 3108105383578700928 20260418.1171 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.3416-00.0466,2461148.6171,13.44,0.05,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 J103.3416-00.0466 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.8511-00.4371,2461148.6171,13.76,0.05,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 J100.8511-00.4371 20260418.1171 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 3109384149958090496,2461148.6171,13.44,0.05,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 3109384149958090496 20260418.1171 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106781193617128320,2461148.6171,13.68,0.05,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
Gaia DR3 3106781193617128320 20260418.1171 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
target,2461148.6171,13.88,0.05,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
target 20260418.1171 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 J107.2145+00.8666,2461148.6171,13.58,0.05,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 J107.2145+00.8666 20260418.1171 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6171,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1171 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461148.6171,13.61,0.05,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 J104.6381-01.6369 20260418.1171 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 J099.7719+00.5391,2461148.6171,13.65,0.05,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 J099.7719+00.5391 20260418.1171 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,2461148.6171,13.74,0.05,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 20260418.1171 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 J106.4222-03.0725,2461148.6171,13.56,0.05,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 J106.4222-03.0725 20260418.1171 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7359+01.8918,2461148.6171,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.7359+01.8918 20260418.1171 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
Gaia DR3 3106319433092617216,2461148.6171,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106319433092617216 20260418.1171 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113071460980262528,2461148.6171,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113071460980262528 20260418.1171 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461148.6171,13.74,0.05,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 20260418.1171 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 J103.6277-01.7188,2461148.6171,13.79,0.05,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 J103.6277-01.7188 20260418.1171 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
Gaia DR3 3107795694950301824,2461148.6171,13.70,0.05,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 3107795694950301824 20260418.1171 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,2461148.6171,13.71,0.05,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 20260418.1171 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 3106915398453298304,2461148.6171,13.72,0.05,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
Gaia DR3 3106915398453298304 20260418.1171 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
ZTF J065124.22+021948.2,2461148.6171,13.56,0.05,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 J065124.22+021948.2 20260418.1171 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.5697-00.9755,2461148.6171,13.79,0.05,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 J099.5697-00.9755 20260418.1171 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
target,2461148.6171,13.80,0.05,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 20260418.1171 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
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
AG Mon,2461148.6171,10.25,0.05,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
AG Mon 20260418.1171 10.25CV 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
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,2461148.6171,10.69,0.05,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
RR Mon 20260418.1171 10.69CV 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 3059510646121751936,2461148.6171,12.49,0.05,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 3059510646121751936 20260418.1171 12.49CV 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
## 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: 2461148.61748100 18.04.2026 02:49:00.358 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
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: 10 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): 35460
Objects passed selection criteria: 35419
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 32365.2
Average stars matched: 31390.2 (96.9875 %)
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 Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 21:53:36 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: 2461148.61748100 18.04.2026 02:49:00.358 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 532
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: 340 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): 248824
Objects passed selection criteria: 248244
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 229684
Average stars matched: 221021 (96.2285 %)
Memory usage VmPeak: 2051184 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 22:02:22 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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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: 2461148.61673056
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Image size: 941.4'x626.8' 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: 06:51:20.828 -01:57:30.59 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 06:51:20.828 -01:57:30.59
Angular distance between the image centers 0.1035 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
Image size: 941.4'x626.9' 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: 06:51:18.865 -01:58:11.78 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 06:51:18.865 -01:58:11.78
Angular distance between the image centers 0.1067 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 06:51:20.828 -01:57:30.59
Second-epoch second image center 06:51:18.865 -01:58:11.78
Angular distance between the image centers 0.01406 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.50GPRbLSnc
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.oPeZCOxnDT
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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits &> /tmp/tmp.R0i7KAwQ98
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits &> /tmp/tmp.tjHfv5AWOH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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 23 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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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
14.7 mag. fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
14.7 mag. fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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.50GPRbLSnc (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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.oPeZCOxnDT (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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.R0i7KAwQ98 (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3088, passed=28741
Got 28741 stars (including 25617 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat
util/solve_plate_with_UCAC5 got 28741 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 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(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 27358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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(), 27356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 27357 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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.tjHfv5AWOH (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_21-49-00_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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3136, passed=28525
Got 28525 stars (including 25360 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 28525 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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 27031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 27026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 27026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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
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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53586.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52512_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52512_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:30.98 +02:01:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52513_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52513_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:33.48 -00:49:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52515_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52515_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:51.47 -05:31:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.957 3100584861478878976 100.46416783203 -05.52409922734 12.0751 11.7375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52520_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52520_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:56.03 -03:45:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.590 3102730592781122176 103.23306216824 -03.75253037047 11.1851 10.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52521_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52521_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:08.54 -01:28:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 2.829 3106909218001458560 099.53605034664 -01.47152094130 11.0094 10.4057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52523_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52523_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:16:54.96 -06:19:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.54, MAG_FAINT_SEARCH_LIMIT=10.52)GAIADR2_OUTPUT=# 0.378 3058236891958149760 109.22900585891 -06.33191038881 9.5741 9.2658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52885_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52885_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:13.70 -02:21:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.161 3108413487348260096 107.30715778798 -02.35884166817 12.0218 10.2260 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52975_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 52975_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:31.30 +01:05:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.534 3111748198735945984 109.38142228257 +01.09484165755 10.3371 8.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53254_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53254_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:58.60 +00:57:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 2.306 3125630563829023488 101.24400728112 +00.95149061823 11.6686 11.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53363_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53363_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:47.52 -05:17:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.114 3100694670902364416 101.19783487843 -05.29681766536 10.3253 8.7996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53463_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53463_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:55:01.59 -02:35:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.791 3105971880037872256 103.75633707660 -02.58618377942 11.9457 11.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:48.26 -04:51:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.785 3102075039031005056 103.20101982134 -04.85629740185 12.0596 11.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:58:50.46 -03:23:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.481 3102669703022235904 104.71018543495 -03.39740832957 12.4647 11.6664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53478_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53478_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:23:29.34 -02:44:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53508_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53508_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:59.22 -05:10:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53530_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53530_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:27:09.38 -03:05:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53544_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53544_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:05:15.98 -04:50:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.957 3101486357939094912 106.31642168106 -04.84271369638 11.9818 11.2815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53550_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53550_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:41.35 +00:00:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53566_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53566_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:50.44 -04:41:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.906 3059308267260336000 108.70995271486 -04.69945687364 11.8823 11.1128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:55.05 -05:39:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.794 3053138078580440064 107.72927321043 -05.65857123656 12.0165 11.3252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:33.93 -01:56:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.502 3106820496858111744 100.14121815381 -01.94367711186 12.3579 11.9644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53586_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 53586_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:36.33 -05:45:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.941 3100562592067548672 100.65113469107 -05.76578883623 12.0773 11.5524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:03:53.14 -06:53:23.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 4s
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 ####
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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Image size: 941.4'x626.8' 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: 06:51:20.828 -01:57:30.59 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 06:51:20.828 -01:57:30.59
Angular distance between the image centers 0.1035 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
Image size: 941.4'x626.9' 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: 06:51:18.865 -01:58:11.78 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 06:51:18.865 -01:58:11.78
Angular distance between the image centers 0.1067 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 06:51:20.828 -01:57:30.59
Second-epoch second image center 06:51:18.865 -01:58:11.78
Angular distance between the image centers 0.01406 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.OG7XC4hz5e
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.ohejQz31Uw
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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits &> /tmp/tmp.6RNUUtknBV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits &> /tmp/tmp.FVGhiANWdT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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 504 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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.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
14.0 mag. fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
14.0 mag. fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OG7XC4hz5e (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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.ohejQz31Uw (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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.6RNUUtknBV (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=30990, passed=204688
Got 204688 stars (including 173459 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat
util/solve_plate_with_UCAC5 got 204688 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 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 196992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 196991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 196985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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.FVGhiANWdT (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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_21-49-00_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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=65, blended=30679, passed=206158
Got 206158 stars (including 175204 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat
util/solve_plate_with_UCAC5 got 206158 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 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: 934 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 199211 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 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: 934 matched stars entering correct_measured_positions(), 199211 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 199208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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
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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/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_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-47-55_20.00sec_-4.90C_LIGHTs_0028.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_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_2026-04-17_CI_Mon-02-Q1b1x1_215003_TTUQ1b1x1_357500_5kTm643o/wcs_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out165339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288525.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288775.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out121122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63434.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 256s
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: 146s
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Considering the candidate 288253_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288253_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288255_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288255_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:39.55 +02:45:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.856 3115241214036930432 108.41420161627 +02.76237003480 14.5648 14.0599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288257_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288257_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:37.12 +01:32:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.865 3114088543597514240 103.15426503193 +01.54525443398 14.7473 14.0804 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288260_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288260_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:02:59.81 +02:14:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.639 3115581444167631232 105.74880032372 +02.23716638684 14.4330 13.8658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288268_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288268_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:45:13.20 -00:39:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.476 3107376991480506624 101.30454362952 -00.65848977728 14.5255 14.0770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288271_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288271_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:23.55 +02:28:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.223 3126484785582824064 102.59778536423 +02.47009934797 14.7160 13.9392 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288280_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288280_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:59:24.77 -00:31:34.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288286_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288286_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288288_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288288_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288296_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288296_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:39:57.18 -00:55:01.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288297_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288297_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288299_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288299_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:25.27 -00:33:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288311_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288311_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:02:21.08 -00:52:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.070 3112564521699860224 105.58811934046 -00.88091558281 14.4819 13.8603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288314_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288314_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:00.30 +01:04:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.190 3113990382121772800 103.25074568869 +01.07648281563 14.3558 13.8349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:00.53 +02:09:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288320_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288320_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:57.11 +00:53:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.588 3111401375834450304 108.48746573778 +00.88308743944 14.3137 13.8628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288326_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288326_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:54:14.80 +03:03:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288331_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288331_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:34:57.22 -00:43:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288332_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288332_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288336_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288336_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:01:19.93 -00:56:40.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288338_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288338_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288343_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288343_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288346_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288346_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288356_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288356_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:23.61 +01:30:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.324 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288364_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288364_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:47.87 +01:17:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.522 3114663832994251776 106.94985792345 +01.29551903786 14.4202 14.1222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288371_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288371_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288373_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288373_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288378_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288378_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:39.22 +02:06:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288388_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288388_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288390_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288390_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288393_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288393_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:04.91 +00:16:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.005 3113556418627340160 102.52022265106 +00.27669937215 14.2226 13.2762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:08:22.39 -05:32:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.986 3053340599185309824 107.09300747588 -05.54396697811 14.2908 14.0677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288403_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288403_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288409_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288409_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:02:12.65 -04:22:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.176 3101742406704701312 105.55273884360 -04.36882587785 14.2554 13.7313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288410_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288410_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:57:45.68 -04:35:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.194 3101676264206730240 104.43986579872 -04.59978271368 14.2028 13.8431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288415_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288415_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288417_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288417_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:11.95 +00:34:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288418_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288418_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 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 288421_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288421_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288434_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288434_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:00:26.18 -01:14:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.781 3112171583731862912 105.10955329640 -01.24825779821 14.0990 13.4064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288436_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288436_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:09.35 +00:44:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.154 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288438_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288438_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:48.87 +00:23:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.756 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288439_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288439_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:05.11 +00:08:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.955 3120076178979162880 098.02062826173 +00.14371115476 14.1568 13.5280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288440_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288440_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:29:25.98 +00:55:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288442_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288442_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:11.96 +00:06:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.118 3111242152807323776 107.29916214691 +00.09921903946 14.1644 13.3350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288443_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288443_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:37:47.08 +02:22:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288444_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288444_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:16:25.89 +01:11:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.593 3111763699275254528 109.10783107228 +01.18558616125 14.1739 13.3905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288453_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288453_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:22.36 +02:05:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.633 3126752482304466432 099.59278061165 +02.09716120278 14.2859 13.6326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288459_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288459_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288464_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288464_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:57.94 +00:32:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.395 3113765669433882752 103.49094480900 +00.53598510870 14.1239 13.7818 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 288468_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288468_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:37:56.03 +00:48:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:05.91 -00:56:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.352 3110870002483448064 108.27457268492 -00.93492738457 14.1042 13.6373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288475_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288475_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:06:19.26 +01:07:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288476_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288476_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:24.16 +01:57:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288477_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288477_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:34:07.95 +01:32:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.072 3120869064303609600 098.53232379767 +01.53750664241 14.1363 13.4916 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 288480_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288480_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:01.06 +01:29:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288496_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288496_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:02.74 -03:47:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288497_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:29:54.08 +03:09:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.328 3124296963600786048 097.47492007358 +03.15619664476 14.0357 13.2323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288498_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288498_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:34.04 -00:32:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.541 3113254602686605824 103.39171426999 -00.53578205621 14.1855 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288501_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288501_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:49.59 +00:06:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.572 3119507765829362176 100.70603017428 +00.10767808842 14.2866 13.9258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288504_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:26.11 +00:51:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288506_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288506_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288507_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288507_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288508_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288508_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288511_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288511_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288514_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288514_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:49:53.39 +01:01:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.634 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 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 288515_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288515_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288519_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:31:44.51 +02:37:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288525_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288525_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:04:08.42 +01:01:42.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 288528_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288528_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288530_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288530_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:57.35 -03:17:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.275 3060069713422807296 109.73872149105 -03.29004521166 13.9133 13.2895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288531_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288531_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288534_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288534_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:19.20 +00:32:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.458 3111506035597560064 109.57968980214 +00.54547492736 13.8524 12.8928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288544_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288544_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:22:24.27 +01:51:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288554_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288554_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:44.75 -06:32:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.478 3052268059949126528 107.68596674381 -06.54594956242 14.1177 13.4542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288556_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288556_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288560_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288560_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:02:53.12 +01:22:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.375 3114623494660947456 105.72108090854 +01.36853343696 14.0378 13.5123 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 288561_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288561_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288566_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288566_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:26:57.22 +02:38:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.639 3124253842129582976 096.73766408759 +02.64412987822 13.6672 12.6389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288567_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288567_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288568_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288568_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:08:42.60 -04:47:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288581_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288581_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:22:19.46 +02:21:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288583_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288583_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:05.58 +02:16:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288589_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288589_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:15:20.36 -02:13:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288591_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288591_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:36:49.49 +02:12:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.517 3126934485838350208 099.20567366977 +02.20587663631 13.9007 13.1385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288593_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288593_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288594_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288594_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 288596_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288596_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288608_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288608_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:35.75 -04:37:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.036 3059498173536851072 108.14873398337 -04.61938055361 13.8382 13.1662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288611_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288611_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288619_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288619_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:16:18.98 -02:34:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.041 3108216125013566848 109.07917314691 -02.58278192350 13.8307 13.4566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288622_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288622_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:00:06.95 +02:57:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.592 3115877826971729792 105.02857894626 +02.96449349911 13.9092 13.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288624_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288624_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:11.74 -02:02:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288626_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288626_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288629_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288629_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:40.34 +01:18:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 5.058 3114487735035278976 107.66741265705 +01.30323744281 13.8264 13.3666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288631_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288631_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:05:27.58 -01:00:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.581 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 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 288633_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288633_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:26.76 -04:20:12.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 288635_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288635_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288640_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288640_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288644_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:49.00 +03:11:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288647_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288647_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288659_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288659_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:08:32.53 -04:52:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.887 3059428423269301248 107.13498037393 -04.87093591462 13.8481 13.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288661_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288661_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:00:52.21 +01:33:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.709 3115389132712944384 105.21749876504 +01.55266609547 13.3442 12.3040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288662_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288662_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 288664_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288664_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:31:48.04 -00:35:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.974 3119256626203802880 097.94986559533 -00.58771369680 13.3413 12.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288667_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288667_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288668_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288668_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288669_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288669_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288672_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:01.87 +00:03:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.438 3111202810908018432 107.75743753981 +00.06395802188 13.6799 13.2216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288673_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288673_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288676_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288676_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:56.72 -06:44:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.153 3052168004389877888 107.73519609496 -06.73692935802 13.6319 12.6605 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288682_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288682_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:37.57 -02:21:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288684_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288684_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:15:07.69 -03:19:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288687_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288687_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288698_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:08.16 -03:40:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288703_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288703_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:36.93 +01:52:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288704_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288704_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288706_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288706_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:11.61 -00:21:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288712_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288712_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:24.50 +00:13:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288715_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288715_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:20.78 -00:46:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.048 3109623190655283968 106.83616090144 -00.78220607274 13.4448 12.9601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288718_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288718_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288720_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288720_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:28.23 +02:18:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288726_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288726_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:33.36 -02:20:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288727_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288727_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:32.31 -04:43:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288729_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288729_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:52.41 -01:20:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.873 3110091239013106560 108.71809649682 -01.33416444841 13.5401 13.0835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288736_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288736_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288737_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288737_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288738_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288743_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288743_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:41.49 -00:55:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288744_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288744_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:31.88 -01:39:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.557 3106879595607559680 099.63337143534 -01.65868987318 11.4562 10.0112 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288747_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288747_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:21:46.42 -01:02:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288748_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288748_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:54.46 +00:41:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288754_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288754_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:42.61 +01:10:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288755_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288755_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:48.77 -02:58:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288758_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288758_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:16.47 -02:07:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.699 3108444995228839296 107.81831127898 -02.12859756211 13.5607 13.0872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288765_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288765_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288769_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288769_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:49:46.87 -00:33:12.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288772_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288772_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288775_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288775_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:51:28.88 +01:57:03.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 288776_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288776_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288780_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288780_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:57:27.89 -01:45:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.571 3112044139160625024 104.36522484805 -01.75663240647 13.3959 12.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288784_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288784_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:42.04 -01:47:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288793_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288793_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:16.59 +00:21:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288795_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288795_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:08:33.16 +00:32:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.858 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:01:35.73 -06:31:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288801_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288801_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:42.21 -02:01:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.729 3108458739123377024 107.42547995682 -02.02695274042 13.3539 12.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288804_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:01.69 -02:44:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288805_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288805_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:09.75 -03:38:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.962 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288808_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:21:33.18 -02:10:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288810_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:16:04.54 +00:48:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288811_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288811_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:51.81 -06:26:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.984 3058010568661382272 109.96562325016 -06.44398460851 13.0319 12.5161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288812_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288812_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288813_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288813_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:57:23.49 +03:02:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 3.775 3127812888253132416 104.34736587287 +03.04555494501 13.2388 12.6552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288814_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:43.68 -02:48:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288816_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288816_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:17.48 -01:16:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288819_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288819_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288820_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:09.25 +00:52:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288823_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:17.32 -01:27:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288825_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288825_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288827_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288827_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:55:46.01 +02:36:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.769 3127768293610081152 103.94127315085 +02.61504769689 12.8271 12.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288828_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288828_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:45.20 -01:18:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288829_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288829_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:09.88 +01:52:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288833_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288833_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:02.36 -01:55:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.731 3109811997422651392 109.25974482713 -01.92788937551 12.8310 12.5097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288835_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:02:05.18 -03:10:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.395 3108637100527185024 105.52093776583 -03.18124398695 12.9536 12.2166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288843_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288843_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:54:08.23 -05:53:00.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 288845_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288845_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288846_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288846_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:20:33.75 -04:55:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288850_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288850_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288852_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288852_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:50.80 +01:53:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288854_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288854_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:56:14.06 -05:00:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288856_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288856_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 288857_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288857_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:01.01 -00:19:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288860_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288860_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:44.68 +02:19:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288863_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288863_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:25:38.47 +01:09:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.607 3123444670289907840 096.40986661190 +01.16585815077 12.2700 11.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288865_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288865_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:17.82 +01:47:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288870_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 288870_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:03.54 -04:55:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288875_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 288875_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 289045_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 289045_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:26:19.79 +03:08:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.44, MAG_FAINT_SEARCH_LIMIT=10.42)GAIADR2_OUTPUT=# 0.383 3124334312636235264 096.58244819334 +03.14356074492 10.2700 9.9385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289685_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 289685_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 289965_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 289965_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:11.48 -02:19:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290000_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 290000_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 290016_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 290016_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290130_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 290130_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 290189_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290189_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:41.64 -00:33:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290199_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290199_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:27.29 +02:30:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.887 3127192557534558720 101.11392637967 +02.51524587168 12.3802 11.9793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290257_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290257_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:29:09.53 -05:33:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290315_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 290315_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290323_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290323_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:53.76 +02:20:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290401_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290401_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:54.74 +02:22:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290527_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290527_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:11.72 -01:59:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290605_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290605_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:03:21.65 -04:07:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.696 3101775525191969408 105.83967354142 -04.12738694134 12.8115 11.9175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290606_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 290606_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290633_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290633_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:41.20 +00:46:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290661_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290661_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:38.41 +01:13:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290705_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290705_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:37.51 +03:12:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.235 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290707_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290707_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:22:45.48 -02:10:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290749_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290749_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:17.14 -00:11:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.259 3121734483032022144 095.32070803228 -00.20016618751 12.9368 12.0752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290762_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290762_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:27:18.50 -05:24:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 3.731 3104187235226900352 096.82605277859 -05.40836792737 12.8062 12.3343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290764_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290764_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:27:08.99 +00:16:35.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290779_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290779_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:39.50 -01:31:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 3.388 3106905262331173632 099.66491829980 -01.52429610039 12.4571 11.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290842_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290842_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:45.66 +02:21:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290955_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290955_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:15:55.63 -06:13:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290960_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290960_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 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 290961_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 290961_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:26.48 +01:43:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291061_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291061_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:35:16.35 -04:45:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.172 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291090_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291090_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:21.65 +03:13:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.912 3127346321664382336 101.84005200571 +03.22712305919 13.0089 12.5860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291127_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291127_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:26:13.00 -01:34:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291140_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291140_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291173_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291173_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291270_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291270_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:13.67 +01:34:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 2.068 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291273_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291273_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:26:20.81 -03:09:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.118 3117129075501324160 096.58656414943 -03.16615954689 13.2570 12.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291412_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291412_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:07.42 +03:13:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 3.297 3127311648388618880 101.03050410819 +03.21757088990 13.2680 12.7484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291432_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291432_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291447_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291447_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:08.98 +02:20:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291459_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291459_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291465_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291465_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:31:45.02 -05:21:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291468_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291468_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291477_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291477_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:17.59 -04:25:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291489_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291489_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:52.30 +01:55:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291569_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:00:51.59 -03:52:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.990 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291580_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291580_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:16.78 -00:38:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291592_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291592_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291622_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291622_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:03.41 -02:29:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 3.927 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291630_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291630_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:12.86 -04:31:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.734 3059503293138179072 108.55373641841 -04.53219512048 13.4465 12.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291684_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291684_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:19.10 +02:16:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.112 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291698_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291698_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:59.17 -01:54:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291750_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291750_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291765_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291765_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291788_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291788_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:22:26.77 -01:42:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 2.716 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291853_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291853_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291875_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291875_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:23:57.57 -04:42:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291885_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291885_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:20:44.62 -02:33:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291899_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291899_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291941_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 291941_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:26.57 -01:03:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.589 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 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 291973_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291973_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 291984_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 291984_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292011_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292011_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:48:31.72 -04:05:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292016_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292016_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292018_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292018_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292027_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:26.10 -06:06:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.210 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292057_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292057_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292063_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292063_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292106_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292106_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292108_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292108_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:55.75 -06:36:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292118_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292118_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292134_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292134_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:18.62 -00:51:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292147_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292147_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292158_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292158_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:10:06.22 +01:43:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.391 3114519998829575296 107.52537717806 +01.72760034637 13.5809 13.0823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292163_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292163_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:41.77 +01:49:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292175_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292175_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:10.40 -05:37:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292194_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292194_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:29:29.76 -00:06:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292217_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292217_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292218_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292218_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:16:34.69 -01:08:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292224_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292224_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:39.17 -02:16:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292228_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292228_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:55.15 -02:23:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292241_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292241_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:11.69 +03:13:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.310 3127311480888772096 101.04831658328 +03.21883456912 13.4524 12.9837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292253_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292253_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292265_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292265_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292267_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292267_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:22:10.54 +00:08:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292277_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292277_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292300_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292300_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 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 292317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292323_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292323_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292329_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292329_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:59.70 -02:44:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292343_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292343_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292374_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292374_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:04:35.28 +02:44:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.232 3115638962369103616 106.14639238151 +02.74839410305 13.5299 12.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292396_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292396_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292401_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292401_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:06:37.21 -04:38:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.338 3101496459701712640 106.65476195883 -04.63532880131 13.6813 13.0848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292409_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292409_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292418_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292418_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292443_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292443_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292456_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292456_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:21:06.66 -03:14:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.372 3059901071527241728 110.27785224367 -03.24709950855 13.5191 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:31:36.92 +00:48:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.587 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292472_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292472_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:45.29 -05:40:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.396 3059140419940666240 107.93738751668 -05.66997036834 13.7391 13.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292563_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292563_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292614_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292614_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:24:33.40 -01:26:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292621_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292621_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:48:33.34 +01:51:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 3.013 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292624_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292624_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:08:00.15 -00:57:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.662 3109605181852110976 107.00017650752 -00.95349251268 13.5091 12.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292629_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292629_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:59:37.45 -00:31:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 5.773 3112646160437322112 104.90516011811 -00.52192288748 13.4503 12.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292649_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292649_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292651_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292651_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:24.08 +02:39:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292693_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292693_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:21:58.09 +01:31:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292728_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292728_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292730_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292730_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292732_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292732_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:54:59.78 +00:10:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.399 3113319370792412800 103.74872486234 +00.18032112282 13.8383 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:39:32.30 +03:12:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.237 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292787_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292787_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:20:25.45 -01:40:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292807_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292807_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292818_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292818_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292840_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292840_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:54:59.58 -01:03:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.020 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292852_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292852_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:22:43.55 -02:10:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292862_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292862_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292889_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292889_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:53.42 +03:13:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.771 3127291139925000832 100.97237071891 +03.21786171975 13.5859 12.7087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292910_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292910_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292944_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292944_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 292947_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292947_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:36.95 -04:25:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292954_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292954_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:49:53.12 +02:30:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.077 3126395102368111488 102.47096542506 +02.50276227856 13.8035 13.2960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292961_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292961_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:27:32.60 +01:54:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292972_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 292972_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:48:53.18 +01:49:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.931 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292983_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 292983_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293007_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293007_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:39.97 +01:31:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293034_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293034_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:54.67 +00:45:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.456 3111384127245493376 107.97730601618 +00.76008378136 13.7155 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293036_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293036_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:43.63 -05:59:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293037_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293037_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:46:37.20 +02:26:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.684 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293051_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293051_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:21:21.18 +01:51:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293097_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293097_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293129_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293129_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293224_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293224_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:28:14.86 +01:53:13.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293227_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293227_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293228_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293228_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293259_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293259_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:29.18 -03:39:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293293_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293293_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293314_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293314_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:46:20.36 -05:15:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.236 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293320_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293320_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293324_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293324_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293336_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293336_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293348_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293348_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:51:34.31 -01:39:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293367_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293367_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293368_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293368_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293388_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293388_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:51:26.38 -02:20:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.048 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293390_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293390_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293442_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293442_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:24.92 +02:10:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.835 3115014508482312960 108.60317000965 +02.16961040523 13.8297 13.2056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293446_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293446_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:27.47 -05:04:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293465_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293465_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293470_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:21.03 -01:43:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293474_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293474_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293494_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293494_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:46.60 -06:52:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293504_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293504_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:03:48.40 -06:03:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293505_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293505_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293510_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293510_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:55.53 -05:04:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.747 3100716802874635136 100.98061063149 -05.06745965125 14.0739 13.7942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293516_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293516_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293517_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293517_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:26.02 -01:49:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293528_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293528_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:39:08.69 -03:48:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.380 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293540_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293540_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293573_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293573_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:46.98 +01:14:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.547 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293584_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293584_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:42:21.43 -01:26:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.724 3107229210246632576 100.58833374413 -01.44282481171 14.1286 13.1420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293590_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293590_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293601_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293601_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:30:07.20 -02:39:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.196 3117217616247602048 097.52997534566 -02.66519300427 14.0065 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293611_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293611_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293614_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293614_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293623_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293623_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:01:28.06 -05:15:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.877 3101401729901841408 105.36605808833 -05.25268963173 13.9656 13.5006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293631_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293631_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:35:42.06 +03:11:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.276 3130161170208610688 098.92490276050 +03.18629758406 13.7622 13.1813 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 293644_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293644_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:26:45.24 -01:30:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293667_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293667_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:04:29.93 -03:50:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.811 3107792709956047232 106.12420013624 -03.83445704157 13.8185 13.3765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293674_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293674_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:18:39.14 -01:16:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293679_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293679_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:03:39.63 -00:16:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.387 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#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 293705_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293705_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293707_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293707_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:52:27.53 -05:52:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293711_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293711_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:24:34.69 -01:26:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.667 3118345204080317440 096.14433564545 -01.44191423101 14.0041 13.5311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293734_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293734_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293743_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293743_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293744_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293744_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293768_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293768_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293781_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293781_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:50.52 +02:53:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.117 3126481555767188608 101.96003040038 +02.88890140059 13.2729 11.9536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:01:15.78 -02:12:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.558 3109049589185408896 105.31471997974 -02.21526180554 13.8444 12.8572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293822_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293822_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293831_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293831_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:51:12.73 +03:05:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.449 3126544605886822656 102.80279501559 +03.08515746517 14.0232 13.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293845_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293845_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293892_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293892_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293899_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293899_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:58:20.41 -00:32:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.113 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293930_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293930_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293949_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293949_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:54:17.82 -04:54:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.433 3102036148108303488 103.57398469743 -04.91417479959 14.1319 13.6028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293958_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293958_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:59.48 -01:17:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.439 3109402463697854208 106.99712734962 -01.29469944657 14.0994 13.3463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293960_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293960_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293985_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 293985_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 293990_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 293990_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:46:34.54 +03:13:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.693 3127256196070019456 101.64373414961 +03.22763545724 13.9846 13.3785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294053_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294053_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:02.90 +01:17:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.617 3114067687234902528 103.26150189626 +01.29007914832 14.2536 13.7674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294061_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294061_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:28.89 -06:01:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294076_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294076_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294107_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294107_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:42.04 -06:20:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.362 3053036859096886656 107.42497549864 -06.33624383095 12.7148 10.9654 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294120_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294120_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:57:27.70 -05:05:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294126_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294126_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:52.51 +01:12:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294250_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294250_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294268_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294268_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294276_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294276_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294281_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294281_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294305_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294305_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294310_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294310_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:46:13.25 +00:50:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.166 3125567827244921728 101.55524044974 +00.83678768778 13.7948 12.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294319_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294319_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294328_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294328_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294395_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294395_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294411_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294411_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294474_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294474_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294499_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294499_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:43:39.50 -04:14:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.234 3105309840899796992 100.91404276516 -04.24696846366 14.4008 13.8045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294513_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294513_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294551_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294551_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294553_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294553_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:57.56 -02:23:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.840 3117243768307728000 098.23916846949 -02.38794555937 14.2908 12.8599 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 294559_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294559_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294570_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294570_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294612_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294612_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294660_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294660_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294678_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294741_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294741_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:46:39.55 -05:23:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.878 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294758_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294758_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:25.04 +00:43:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294760_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:59:42.43 +00:17:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.733 3112951201897467136 104.92679471042 +00.29040761527 14.3636 13.5626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294762_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294762_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:14:12.04 -05:29:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.690 3059111489041433600 108.54938650423 -05.49003020592 14.3245 14.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294766_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294766_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294785_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294785_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294798_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294798_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:43.53 -01:58:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294799_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:22.47 +01:18:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.135 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294803_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294803_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:17:46.39 -04:14:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.761 3059716598390959232 109.44252754145 -04.23844785020 14.3995 13.6406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294834_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294834_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294844_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294844_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:38:31.38 +02:25:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.939 3126956441710853888 099.63043614299 +02.42681295214 14.2095 13.6254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294866_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294866_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294868_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294868_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294876_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294876_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294898_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294898_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:41:04.21 +02:37:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294917_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294917_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294957_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294957_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:47.96 +00:29:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.701 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294994_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 294994_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 294999_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 294999_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:59:12.07 -02:20:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.806 3108997293662134400 104.79962658383 -02.33451681197 14.6167 14.2326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295006_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295006_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295026_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295026_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295036_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295036_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295073_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295073_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295088_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295088_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:25:45.39 -04:57:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295120_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295120_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:38.60 -04:08:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295127_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295127_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:37:41.96 -02:45:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.813 3106462575761447552 099.42437960667 -02.76637400626 14.5622 14.1305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295138_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295138_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:09.07 -04:07:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.024 3107534152928192512 107.28726652518 -04.13143194844 14.3172 14.0151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295205_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295205_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295208_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295208_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:16.64 -05:04:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.802 3053426017496460416 106.81884344475 -05.08354785989 14.3438 13.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295209_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295209_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295226_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295226_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:09.54 -03:03:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.582 3108135517070218624 107.78905019836 -03.06566155718 14.3689 13.5789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295233_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295233_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:17.98 -04:51:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.929 3059404989926960896 107.82440417551 -04.86285565371 14.2314 13.6329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295237_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295237_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:27.87 -02:41:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295247_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295247_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:00:20.17 +01:48:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.430 3115456202921062528 105.08373232209 +01.80654312181 14.5496 13.9285 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 295266_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295266_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295283_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295283_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:04:34.50 -02:58:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.035 3108656612557076480 106.14297456909 -02.97561603727 14.4140 13.7650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295287_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295287_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:01:16.95 -03:08:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.769 3108641601653031808 105.32017771023 -03.14933571605 14.6041 14.1402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295294_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295294_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295305_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295305_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295317_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:39:24.15 +00:43:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.498 3119835523372503168 099.85053919624 +00.72058909907 14.4464 13.3750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295318_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295318_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295329_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295329_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:48:38.17 +02:13:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.022 3126383523135600000 102.15899293903 +02.22816190581 14.4895 13.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295330_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295330_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:59.34 +01:34:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295346_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295346_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
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Considering the candidate 295361_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295361_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:56.72 +02:19:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.682 3126200355668642688 102.73585150791 +02.31838588562 14.6908 14.0766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295372_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295372_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295375_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295375_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:21:46.41 -03:41:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.573 3116816814198300544 095.44366963076 -03.68796221192 14.5373 13.9496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295378_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295378_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295380_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295380_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:20:35.92 -03:26:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.872 3059873519315313792 110.14909195384 -03.44590985835 14.3776 13.6570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295396_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295396_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:11:21.78 +00:01:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.821 3111199615451706752 107.84032222228 +00.01800070644 14.5208 13.9880 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 295400_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295400_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295410_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295410_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295422_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295422_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295437_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295437_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295467_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:23:27.20 +02:43:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.561 3124948115002957824 095.86299834490 +02.71714997212 14.4245 13.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295475_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295475_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:17.01 +01:00:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295488_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295488_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:44:39.32 -01:38:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.629 3107031263793230720 101.16315248394 -01.64775762578 14.4751 13.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295493_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295493_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:13:48.96 -00:33:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.453 3110921125473181184 108.45302386624 -00.56062074070 14.5209 14.0641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295495_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295495_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:11.90 -05:41:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295496_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295496_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:45.39 +01:59:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.893 3126206162465063296 103.43878066168 +01.99257415158 14.6770 14.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295527_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295527_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295564_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295564_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:32:16.18 -02:12:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.523 3117263078480669696 098.06643809547 -02.20517777006 14.6833 14.1307 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295579_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295579_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:07:55.14 -02:17:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.112 3109174929210280320 106.97938927799 -02.28619493009 14.7216 13.9160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295582_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:47:11.58 +01:55:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.558 3125972825481614848 101.79839570905 +01.92014812407 14.6887 14.1602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295592_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295592_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295595_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295595_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295600_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295600_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:05:22.79 -01:37:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.524 3109462966898813184 106.34401149466 -01.61788220358 14.4979 13.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295602_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:06:58.17 +02:05:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.202 3114788215246409088 106.74201411688 +02.09671466542 14.4155 13.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295632_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295632_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:40:02.61 +01:14:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.961 3125874590987954944 100.01022644423 +01.24177768515 14.1876 13.2032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295634_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295634_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:09:07.34 +00:45:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.779 3114304223971525888 107.28004356478 +00.75325950007 14.6190 14.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295677_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 295677_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:45:47.74 +02:43:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.644 3127202629238414208 101.44922137078 +02.73194274637 14.4937 13.5437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295680_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 295680_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:12:52.13 -05:20:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91187_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 91187_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:29:53.94 -03:35:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 65114_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:27:01.34 -04:35:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:50:00.90 +01:46:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 5.308 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165339_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 165339_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 06:53:07.15 -00:45:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 2.512 3112405603608183680 103.27953662954 -00.75934393491 12.4145 12.1083 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63434_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
Preparing report for the candidate 63434_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:19:38.78 -02:00:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-17_21-49-00_20.00sec_-4.90C_LIGHTs_0029 did not pass the final checks
**** FOUND 07:03:53.14 -06:53:23.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 421s
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 ####
07:09:13.70 -02:21:30.6
07:17:31.29 +01:05:39.2
06:39:53.99 +02:23:22.4
06:39:20.08 +00:23:03.7
07:01:12.34 -00:55:21.7
06:56:14.69 -03:49:56.7
06:43:39.43 +03:05:01.9
06:45:34.10 +03:08:05.6
07:02:02.05 -01:53:45.0
06:36:46.77 +02:28:24.3
06:43:51.27 +03:09:10.1
07:02:53.01 -04:59:09.0
06:51:40.94 -00:36:47.3
06:56:30.70 +01:10:47.6
06:46:56.75 +01:41:48.2
07:12:29.44 -01:56:23.7
07:01:36.99 -04:32:42.3
06:50:45.36 +01:03:08.2
07:03:06.49 -05:17:29.6
06:39:41.67 +01:09:51.9
06:42:00.96 +00:23:10.9
06:48:15.43 -05:22:39.6
06:57:22.85 +02:20:23.7
06:56:04.45 -01:29:59.6
07:21:12.24 -01:21:16.4
07:08:45.88 +01:25:42.4
07:18:22.69 +00:37:20.2
06:41:26.76 +02:47:59.5
07:20:22.44 +01:19:55.4
07:02:23.69 -01:34:41.1
07:00:39.12 -01:30:26.1
07:10:55.07 -00:54:14.1
07:04:32.09 +00:11:21.8
07:11:30.24 +00:31:17.4
07:04:05.58 +00:58:05.8
07:20:34.18 -00:45:32.6
07:08:13.33 -04:47:30.8
06:46:25.57 -00:28:35.9
07:17:31.42 -00:53:39.9
07:02:08.18 +02:42:03.7
06:30:15.28 +02:16:00.3
06:41:58.52 +02:45:41.4
06:33:18.02 +00:28:22.1
07:11:37.57 -06:35:51.4
06:59:35.47 +00:38:55.5
07:19:23.98 -02:42:21.2
07:10:10.13 -00:55:10.3
07:20:41.13 -03:34:37.7
06:43:32.68 +01:24:31.8
07:05:57.75 +02:49:17.9
07:19:37.64 -02:20:15.6
07:21:26.66 -03:34:46.4
06:48:07.75 -00:40:38.3
07:02:33.63 -01:57:58.4
07:06:31.75 +01:08:40.3
07:20:48.34 -06:16:18.5
07:08:17.17 -04:56:00.9
06:57:24.16 -00:50:14.3
07:18:48.76 -01:43:49.2
07:18:31.83 -06:47:04.5
07:07:04.86 -03:10:06.2
07:08:25.19 +02:46:17.6
07:03:36.88 +02:37:11.3
07:14:02.19 -01:05:33.3
07:10:14.40 -00:48:25.3
06:49:26.79 +02:25:16.6
07:12:11.47 -02:24:18.3
07:08:43.53 +01:59:22.8
07:08:24.33 -01:19:54.2
07:05:13.23 -06:04:45.2
07:01:16.10 -02:29:02.8
06:59:38.82 -01:27:09.2
07:13:32.81 +00:13:14.5
07:16:00.07 +01:17:46.5
07:09:57.35 -01:59:05.9
06:57:47.70 -01:31:07.3
06:50:49.69 -01:13:39.2
06:43:27.95 -03:56:28.9
07:17:50.85 -01:41:24.3
06:48:15.54 +01:46:16.6
07:08:35.63 +01:46:44.6
06:40:30.49 -01:04:41.9
06:53:50.85 -00:03:50.8
06:58:08.39 -01:38:49.8
07:09:20.65 +02:38:45.3
07:04:54.61 +00:11:37.3
06:34:11.12 -00:21:48.8
07:17:09.62 +02:29:28.1
07:05:12.17 -03:19:36.5
06:55:39.03 -06:15:20.8
06:41:43.54 -01:05:57.1
06:42:33.27 -03:28:04.5
07:19:08.24 -02:01:49.4
07:15:07.29 +02:40:51.9
07:20:50.33 -00:51:22.7
07:01:14.59 +00:57:29.3
07:16:04.08 +02:09:50.7
07:10:18.71 -01:17:10.7
06:57:38.25 +02:11:06.7
07:15:26.09 -01:11:22.2
06:44:16.61 -00:10:05.4
07:03:04.49 -01:18:37.3
06:43:50.85 +01:35:53.8
07:10:55.84 -00:46:11.3
06:30:03.44 +01:18:36.1
06:56:36.62 +02:42:44.9
06:29:32.93 -02:51:13.6
07:07:33.42 -03:25:31.7
06:57:12.36 -03:57:42.9
07:07:07.01 +01:40:01.5
07:04:16.78 -03:01:36.9
07:06:11.95 +00:18:35.4
06:48:38.13 +02:54:38.4
06:55:03.23 -01:02:51.0
06:54:39.44 +02:38:01.5
06:50:59.53 +00:13:39.9
07:09:29.04 -06:44:33.8
07:11:55.44 -04:52:52.9
06:43:42.50 -04:26:30.0
07:12:39.26 -06:53:46.5
06:35:10.43 -00:43:20.3
07:21:06.36 -03:15:03.6
06:45:05.03 +02:42:58.0
07:07:40.41 -03:15:05.7
07:15:10.17 +00:22:00.4
06:52:06.51 -01:18:21.8
06:35:21.92 -05:17:33.0
06:36:32.34 -03:35:55.8
07:04:51.61 -02:12:04.2
06:50:09.77 -03:29:01.2
06:52:47.86 -06:19:16.7
06:45:33.70 -00:26:17.2
06:46:10.38 -03:13:58.6
06:47:23.66 +01:25:44.1
06:54:44.93 -01:17:25.8
07:05:25.58 -03:18:31.3
06:44:50.77 +01:05:45.2
07:11:11.59 -00:11:47.3
06:53:13.90 -04:35:48.3
07:09:21.64 +01:07:27.2
07:06:54.22 +02:10:49.2
06:45:17.67 +00:43:40.0
06:44:56.87 +01:18:45.6
07:14:23.48 -03:02:01.1
07:02:32.42 -00:13:09.4
06:38:07.57 +03:11:51.7
06:46:32.71 -01:51:13.3
06:47:59.60 -01:20:53.6
06:26:39.13 +00:26:39.7
06:59:49.89 -06:00:37.1
06:35:16.68 -01:19:06.8
06:46:18.39 -02:26:01.6
07:03:46.03 -02:09:32.8
07:03:07.01 +01:49:29.8
06:46:42.26 -05:47:35.3
07:07:03.77 -02:21:52.3
06:38:18.60 -03:21:23.7
06:44:12.58 -00:00:23.8
06:45:39.04 +02:45:22.7
06:47:20.31 +03:13:33.6
06:58:48.17 -00:36:47.5
06:59:10.77 -01:18:50.7
07:05:26.19 +01:29:35.0
07:04:19.80 +00:50:06.0
06:35:27.03 +00:29:41.6
07:17:24.01 +01:22:49.3
06:33:36.46 +02:19:22.9
07:05:42.94 -01:37:20.0
06:44:36.59 +00:59:55.7
06:51:01.05 +02:05:33.2
07:18:26.93 -01:08:11.3
06:53:47.35 -02:38:43.7
06:45:20.36 -01:12:37.2
06:48:04.88 +02:16:48.2
06:41:21.32 -00:35:22.9
06:44:38.19 -02:01:19.8
06:52:39.32 +00:08:53.5
06:21:05.81 -03:21:15.1
06:44:45.21 -04:22:27.7
06:54:49.15 -04:18:03.7
06:48:44.06 +02:01:36.7
06:46:12.27 +00:43:10.4
06:42:37.27 +02:58:09.2
07:21:14.34 +01:37:59.7
06:58:37.43 -06:48:35.7
07:13:18.55 -02:57:58.7
06:53:20.05 -00:02:21.4
06:43:24.84 -00:26:06.9
07:08:57.82 -01:26:26.5
06:39:16.36 -02:19:47.7
06:32:45.42 -00:27:20.1
07:08:53.85 +00:51:37.0
06:44:14.07 +02:30:45.5
06:58:34.51 -01:38:22.4
06:39:06.15 +00:32:10.0
07:02:45.57 -04:03:42.1
07:05:41.39 -03:03:49.3
06:46:55.19 +01:53:18.7
06:48:40.37 -01:40:11.7
07:00:46.17 +00:40:11.7
06:57:39.43 -03:34:42.5
06:54:27.95 -01:43:27.6
07:05:08.88 -03:40:22.2
07:12:27.96 -04:46:31.0
06:39:31.84 -01:20:52.1
06:51:24.01 +02:19:39.4
06:38:16.13 -00:57:51.9
06:44:44.47 +03:07:31.7
07:12:42.41 -04:32:29.3
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:39:53.99 +02:23:22.4
06:39:20.08 +00:23:03.7
07:01:12.34 -00:55:21.7
06:56:14.69 -03:49:56.7
06:43:39.43 +03:05:01.9
06:45:34.10 +03:08:05.6
07:02:02.05 -01:53:45.0
06:36:46.77 +02:28:24.3
06:43:51.27 +03:09:10.1
07:02:53.01 -04:59:09.0
06:51:40.94 -00:36:47.3
06:56:30.70 +01:10:47.6
06:46:56.75 +01:41:48.2
07:12:29.44 -01:56:23.7
07:01:36.99 -04:32:42.3
06:50:45.36 +01:03:08.2
07:03:06.49 -05:17:29.6
06:39:41.67 +01:09:51.9
06:42:00.96 +00:23:10.9
06:48:15.43 -05:22:39.6
06:57:22.85 +02:20:23.7
06:56:04.45 -01:29:59.6
07:21:12.24 -01:21:16.4
07:08:45.88 +01:25:42.4
07:18:22.69 +00:37:20.2
06:41:26.76 +02:47:59.5
07:20:22.44 +01:19:55.4
07:02:23.69 -01:34:41.1
07:00:39.12 -01:30:26.1
07:10:55.07 -00:54:14.1
07:04:32.09 +00:11:21.8
07:11:30.24 +00:31:17.4
07:04:05.58 +00:58:05.8
07:20:34.18 -00:45:32.6
07:08:13.33 -04:47:30.8
06:46:25.57 -00:28:35.9
07:17:31.42 -00:53:39.9
07:02:08.18 +02:42:03.7
06:30:15.28 +02:16:00.3
06:41:58.52 +02:45:41.4
06:33:18.02 +00:28:22.1
07:11:37.57 -06:35:51.4
06:59:35.47 +00:38:55.5
07:19:23.98 -02:42:21.2
07:10:10.13 -00:55:10.3
07:20:41.13 -03:34:37.7
06:43:32.68 +01:24:31.8
07:05:57.75 +02:49:17.9
07:19:37.64 -02:20:15.6
07:21:26.66 -03:34:46.4
06:48:07.75 -00:40:38.3
07:02:33.63 -01:57:58.4
07:06:31.75 +01:08:40.3
07:20:48.34 -06:16:18.5
07:08:17.17 -04:56:00.9
06:57:24.16 -00:50:14.3
07:18:48.76 -01:43:49.2
07:18:31.83 -06:47:04.5
07:07:04.86 -03:10:06.2
07:08:25.19 +02:46:17.6
07:03:36.88 +02:37:11.3
07:14:02.19 -01:05:33.3
07:10:14.40 -00:48:25.3
06:49:26.79 +02:25:16.6
07:12:11.47 -02:24:18.3
07:08:43.53 +01:59:22.8
07:08:24.33 -01:19:54.2
07:05:13.23 -06:04:45.2
07:01:16.10 -02:29:02.8
06:59:38.82 -01:27:09.2
07:13:32.81 +00:13:14.5
07:16:00.07 +01:17:46.5
07:09:57.35 -01:59:05.9
06:57:47.70 -01:31:07.3
06:50:49.69 -01:13:39.2
06:43:27.95 -03:56:28.9
07:17:50.85 -01:41:24.3
06:48:15.54 +01:46:16.6
07:08:35.63 +01:46:44.6
06:40:30.49 -01:04:41.9
06:53:50.85 -00:03:50.8
06:58:08.39 -01:38:49.8
07:09:20.65 +02:38:45.3
07:04:54.61 +00:11:37.3
06:34:11.12 -00:21:48.8
07:17:09.62 +02:29:28.1
07:05:12.17 -03:19:36.5
06:55:39.03 -06:15:20.8
06:41:43.54 -01:05:57.1
06:42:33.27 -03:28:04.5
07:19:08.24 -02:01:49.4
07:15:07.29 +02:40:51.9
07:20:50.33 -00:51:22.7
07:01:14.59 +00:57:29.3
07:16:04.08 +02:09:50.7
07:10:18.71 -01:17:10.7
06:57:38.25 +02:11:06.7
07:15:26.09 -01:11:22.2
06:44:16.61 -00:10:05.4
07:03:04.49 -01:18:37.3
06:43:50.85 +01:35:53.8
07:10:55.84 -00:46:11.3
06:30:03.44 +01:18:36.1
06:56:36.62 +02:42:44.9
06:29:32.93 -02:51:13.6
07:07:33.42 -03:25:31.7
06:57:12.36 -03:57:42.9
07:07:07.01 +01:40:01.5
07:04:16.78 -03:01:36.9
07:06:11.95 +00:18:35.4
06:48:38.13 +02:54:38.4
06:55:03.23 -01:02:51.0
06:54:39.44 +02:38:01.5
06:50:59.53 +00:13:39.9
07:09:29.04 -06:44:33.8
07:11:55.44 -04:52:52.9
06:43:42.50 -04:26:30.0
07:12:39.26 -06:53:46.5
06:35:10.43 -00:43:20.3
07:21:06.36 -03:15:03.6
06:45:05.03 +02:42:58.0
07:07:40.41 -03:15:05.7
07:15:10.17 +00:22:00.4
06:52:06.51 -01:18:21.8
06:35:21.92 -05:17:33.0
06:36:32.34 -03:35:55.8
07:04:51.61 -02:12:04.2
06:50:09.77 -03:29:01.2
06:52:47.86 -06:19:16.7
06:45:33.70 -00:26:17.2
06:46:10.38 -03:13:58.6
06:47:23.66 +01:25:44.1
06:54:44.93 -01:17:25.8
07:05:25.58 -03:18:31.3
06:44:50.77 +01:05:45.2
07:11:11.59 -00:11:47.3
06:53:13.90 -04:35:48.3
07:09:21.64 +01:07:27.2
07:06:54.22 +02:10:49.2
06:45:17.67 +00:43:40.0
06:44:56.87 +01:18:45.6
07:14:23.48 -03:02:01.1
07:02:32.42 -00:13:09.4
06:38:07.57 +03:11:51.7
06:46:32.71 -01:51:13.3
06:47:59.60 -01:20:53.6
06:26:39.13 +00:26:39.7
06:59:49.89 -06:00:37.1
06:35:16.68 -01:19:06.8
06:46:18.39 -02:26:01.6
07:03:46.03 -02:09:32.8
07:03:07.01 +01:49:29.8
06:46:42.26 -05:47:35.3
07:07:03.77 -02:21:52.3
06:38:18.60 -03:21:23.7
06:44:12.58 -00:00:23.8
06:45:39.04 +02:45:22.7
06:47:20.31 +03:13:33.6
06:58:48.17 -00:36:47.5
06:59:10.77 -01:18:50.7
07:05:26.19 +01:29:35.0
07:04:19.80 +00:50:06.0
06:35:27.03 +00:29:41.6
07:17:24.01 +01:22:49.3
06:33:36.46 +02:19:22.9
07:05:42.94 -01:37:20.0
06:44:36.59 +00:59:55.7
06:51:01.05 +02:05:33.2
07:18:26.93 -01:08:11.3
06:53:47.35 -02:38:43.7
06:45:20.36 -01:12:37.2
06:48:04.88 +02:16:48.2
06:41:21.32 -00:35:22.9
06:44:38.19 -02:01:19.8
06:52:39.32 +00:08:53.5
06:21:05.81 -03:21:15.1
06:44:45.21 -04:22:27.7
06:54:49.15 -04:18:03.7
06:48:44.06 +02:01:36.7
06:46:12.27 +00:43:10.4
06:42:37.27 +02:58:09.2
07:21:14.34 +01:37:59.7
06:58:37.43 -06:48:35.7
07:13:18.55 -02:57:58.7
06:53:20.05 -00:02:21.4
06:43:24.84 -00:26:06.9
07:08:57.82 -01:26:26.5
06:39:16.36 -02:19:47.7
06:32:45.42 -00:27:20.1
07:08:53.85 +00:51:37.0
06:44:14.07 +02:30:45.5
06:58:34.51 -01:38:22.4
06:39:06.15 +00:32:10.0
07:02:45.57 -04:03:42.1
07:05:41.39 -03:03:49.3
06:46:55.19 +01:53:18.7
06:48:40.37 -01:40:11.7
07:00:46.17 +00:40:11.7
06:57:39.43 -03:34:42.5
06:54:27.95 -01:43:27.6
07:05:08.88 -03:40:22.2
07:12:27.96 -04:46:31.0
06:39:31.84 -01:20:52.1
06:51:24.01 +02:19:39.4
06:38:16.13 -00:57:51.9
06:44:44.47 +03:07:31.7
07:09:13.70 -02:21:30.6
07:17:31.29 +01:05:39.2
07:12:42.41 -04:32:29.3
###################################################################################
06:39:53.99 +02:23:22.4 -- not an asteroid (will add it to exclusion list)
06:39:20.08 +00:23:03.7 -- not an asteroid (will add it to exclusion list)
07:01:12.34 -00:55:21.7 -- not an asteroid (will add it to exclusion list)
06:56:14.69 -03:49:56.7 -- not an asteroid (will add it to exclusion list)
06:43:39.43 +03:05:01.9 -- not an asteroid (will add it to exclusion list)
06:45:34.10 +03:08:05.6 -- not an asteroid (will add it to exclusion list)
07:02:02.05 -01:53:45.0 -- not an asteroid (will add it to exclusion list)
06:36:46.77 +02:28:24.3 -- not an asteroid (will add it to exclusion list)
06:43:51.27 +03:09:10.1 -- not an asteroid (will add it to exclusion list)
07:02:53.01 -04:59:09.0 -- not an asteroid (will add it to exclusion list)
06:51:40.94 -00:36:47.3 -- not an asteroid (will add it to exclusion list)
06:56:30.70 +01:10:47.6 -- not an asteroid (will add it to exclusion list)
06:46:56.75 +01:41:48.2 -- not an asteroid (will add it to exclusion list)
07:12:29.44 -01:56:23.7 -- not an asteroid (will add it to exclusion list)
07:01:36.99 -04:32:42.3 -- not an asteroid (will add it to exclusion list)
06:50:45.36 +01:03:08.2 -- not an asteroid (will add it to exclusion list)
07:03:06.49 -05:17:29.6 -- not an asteroid (will add it to exclusion list)
06:39:41.67 +01:09:51.9 -- not an asteroid (will add it to exclusion list)
06:42:00.96 +00:23:10.9 -- not an asteroid (will add it to exclusion list)
06:48:15.43 -05:22:39.6 -- not an asteroid (will add it to exclusion list)
06:57:22.85 +02:20:23.7 -- not an asteroid (will add it to exclusion list)
06:56:04.45 -01:29:59.6 -- not an asteroid (will add it to exclusion list)
07:21:12.24 -01:21:16.4 -- not an asteroid (will add it to exclusion list)
07:08:45.88 +01:25:42.4 -- not an asteroid (will add it to exclusion list)
07:18:22.69 +00:37:20.2 -- not an asteroid (will add it to exclusion list)
06:41:26.76 +02:47:59.5 -- not an asteroid (will add it to exclusion list)
07:20:22.44 +01:19:55.4 -- not an asteroid (will add it to exclusion list)
07:02:23.69 -01:34:41.1 -- not an asteroid (will add it to exclusion list)
07:00:39.12 -01:30:26.1 -- not an asteroid (will add it to exclusion list)
07:10:55.07 -00:54:14.1 -- not an asteroid (will add it to exclusion list)
07:04:32.09 +00:11:21.8 -- not an asteroid (will add it to exclusion list)
07:11:30.24 +00:31:17.4 -- not an asteroid (will add it to exclusion list)
07:04:05.58 +00:58:05.8 -- not an asteroid (will add it to exclusion list)
07:20:34.18 -00:45:32.6 -- not an asteroid (will add it to exclusion list)
07:08:13.33 -04:47:30.8 -- not an asteroid (will add it to exclusion list)
06:46:25.57 -00:28:35.9 -- not an asteroid (will add it to exclusion list)
07:17:31.42 -00:53:39.9 -- not an asteroid (will add it to exclusion list)
07:02:08.18 +02:42:03.7 -- not an asteroid (will add it to exclusion list)
06:30:15.28 +02:16:00.3 -- not an asteroid (will add it to exclusion list)
06:41:58.52 +02:45:41.4 -- not an asteroid (will add it to exclusion list)
06:33:18.02 +00:28:22.1 -- not an asteroid (will add it to exclusion list)
07:11:37.57 -06:35:51.4 -- not an asteroid (will add it to exclusion list)
06:59:35.47 +00:38:55.5 -- not an asteroid (will add it to exclusion list)
07:19:23.98 -02:42:21.2 -- not an asteroid (will add it to exclusion list)
07:10:10.13 -00:55:10.3 -- not an asteroid (will add it to exclusion list)
07:20:41.13 -03:34:37.7 -- not an asteroid (will add it to exclusion list)
06:43:32.68 +01:24:31.8 -- not an asteroid (will add it to exclusion list)
07:05:57.75 +02:49:17.9 -- not an asteroid (will add it to exclusion list)
07:19:37.64 -02:20:15.6 -- not an asteroid (will add it to exclusion list)
07:21:26.66 -03:34:46.4 -- not an asteroid (will add it to exclusion list)
06:48:07.75 -00:40:38.3 -- not an asteroid (will add it to exclusion list)
07:02:33.63 -01:57:58.4 -- not an asteroid (will add it to exclusion list)
07:06:31.75 +01:08:40.3 -- not an asteroid (will add it to exclusion list)
07:20:48.34 -06:16:18.5 -- not an asteroid (will add it to exclusion list)
07:08:17.17 -04:56:00.9 -- not an asteroid (will add it to exclusion list)
06:57:24.16 -00:50:14.3 -- not an asteroid (will add it to exclusion list)
07:18:48.76 -01:43:49.2 -- not an asteroid (will add it to exclusion list)
07:18:31.83 -06:47:04.5 -- not an asteroid (will add it to exclusion list)
07:07:04.86 -03:10:06.2 -- not an asteroid (will add it to exclusion list)
07:08:25.19 +02:46:17.6 -- not an asteroid (will add it to exclusion list)
07:03:36.88 +02:37:11.3 -- not an asteroid (will add it to exclusion list)
07:14:02.19 -01:05:33.3 -- not an asteroid (will add it to exclusion list)
07:10:14.40 -00:48:25.3 -- not an asteroid (will add it to exclusion list)
06:49:26.79 +02:25:16.6 -- not an asteroid (will add it to exclusion list)
07:12:11.47 -02:24:18.3 -- not an asteroid (will add it to exclusion list)
07:08:43.53 +01:59:22.8 -- not an asteroid (will add it to exclusion list)
07:08:24.33 -01:19:54.2 -- not an asteroid (will add it to exclusion list)
07:05:13.23 -06:04:45.2 -- not an asteroid (will add it to exclusion list)
07:01:16.10 -02:29:02.8 -- not an asteroid (will add it to exclusion list)
06:59:38.82 -01:27:09.2 -- not an asteroid (will add it to exclusion list)
07:13:32.81 +00:13:14.5 -- not an asteroid (will add it to exclusion list)
07:16:00.07 +01:17:46.5 -- not an asteroid (will add it to exclusion list)
07:09:57.35 -01:59:05.9 -- not an asteroid (will add it to exclusion list)
06:57:47.70 -01:31:07.3 -- not an asteroid (will add it to exclusion list)
06:50:49.69 -01:13:39.2 -- not an asteroid (will add it to exclusion list)
06:43:27.95 -03:56:28.9 -- not an asteroid (will add it to exclusion list)
07:17:50.85 -01:41:24.3 -- not an asteroid (will add it to exclusion list)
06:48:15.54 +01:46:16.6 -- not an asteroid (will add it to exclusion list)
07:08:35.63 +01:46:44.6 -- not an asteroid (will add it to exclusion list)
06:40:30.49 -01:04:41.9 -- not an asteroid (will add it to exclusion list)
06:53:50.85 -00:03:50.8 -- not an asteroid (will add it to exclusion list)
06:58:08.39 -01:38:49.8 -- not an asteroid (will add it to exclusion list)
07:09:20.65 +02:38:45.3 -- not an asteroid (will add it to exclusion list)
07:04:54.61 +00:11:37.3 -- not an asteroid (will add it to exclusion list)
06:34:11.12 -00:21:48.8 -- not an asteroid (will add it to exclusion list)
07:17:09.62 +02:29:28.1 -- not an asteroid (will add it to exclusion list)
07:05:12.17 -03:19:36.5 -- not an asteroid (will add it to exclusion list)
06:55:39.03 -06:15:20.8 -- not an asteroid (will add it to exclusion list)
06:41:43.54 -01:05:57.1 -- not an asteroid (will add it to exclusion list)
06:42:33.27 -03:28:04.5 -- not an asteroid (will add it to exclusion list)
07:19:08.24 -02:01:49.4 -- not an asteroid (will add it to exclusion list)
07:15:07.29 +02:40:51.9 -- not an asteroid (will add it to exclusion list)
07:20:50.33 -00:51:22.7 -- not an asteroid (will add it to exclusion list)
07:01:14.59 +00:57:29.3 -- not an asteroid (will add it to exclusion list)
07:16:04.08 +02:09:50.7 -- not an asteroid (will add it to exclusion list)
07:10:18.71 -01:17:10.7 -- not an asteroid (will add it to exclusion list)
06:57:38.25 +02:11:06.7 -- not an asteroid (will add it to exclusion list)
07:15:26.09 -01:11:22.2 -- not an asteroid (will add it to exclusion list)
06:44:16.61 -00:10:05.4 -- not an asteroid (will add it to exclusion list)
07:03:04.49 -01:18:37.3 -- not an asteroid (will add it to exclusion list)
06:43:50.85 +01:35:53.8 -- not an asteroid (will add it to exclusion list)
07:10:55.84 -00:46:11.3 -- not an asteroid (will add it to exclusion list)
06:30:03.44 +01:18:36.1 -- not an asteroid (will add it to exclusion list)
06:56:36.62 +02:42:44.9 -- not an asteroid (will add it to exclusion list)
06:29:32.93 -02:51:13.6 -- not an asteroid (will add it to exclusion list)
07:07:33.42 -03:25:31.7 -- not an asteroid (will add it to exclusion list)
06:57:12.36 -03:57:42.9 -- not an asteroid (will add it to exclusion list)
07:07:07.01 +01:40:01.5 -- not an asteroid (will add it to exclusion list)
07:04:16.78 -03:01:36.9 -- not an asteroid (will add it to exclusion list)
07:06:11.95 +00:18:35.4 -- not an asteroid (will add it to exclusion list)
06:48:38.13 +02:54:38.4 -- not an asteroid (will add it to exclusion list)
06:55:03.23 -01:02:51.0 -- not an asteroid (will add it to exclusion list)
06:54:39.44 +02:38:01.5 -- not an asteroid (will add it to exclusion list)
06:50:59.53 +00:13:39.9 -- not an asteroid (will add it to exclusion list)
07:09:29.04 -06:44:33.8 -- not an asteroid (will add it to exclusion list)
07:11:55.44 -04:52:52.9 -- not an asteroid (will add it to exclusion list)
06:43:42.50 -04:26:30.0 -- not an asteroid (will add it to exclusion list)
07:12:39.26 -06:53:46.5 -- not an asteroid (will add it to exclusion list)
06:35:10.43 -00:43:20.3 -- not an asteroid (will add it to exclusion list)
07:21:06.36 -03:15:03.6 -- not an asteroid (will add it to exclusion list)
06:45:05.03 +02:42:58.0 -- not an asteroid (will add it to exclusion list)
07:07:40.41 -03:15:05.7 -- not an asteroid (will add it to exclusion list)
07:15:10.17 +00:22:00.4 -- not an asteroid (will add it to exclusion list)
06:52:06.51 -01:18:21.8 -- not an asteroid (will add it to exclusion list)
06:35:21.92 -05:17:33.0 -- not an asteroid (will add it to exclusion list)
06:36:32.34 -03:35:55.8 -- not an asteroid (will add it to exclusion list)
07:04:51.61 -02:12:04.2 -- not an asteroid (will add it to exclusion list)
06:50:09.77 -03:29:01.2 -- not an asteroid (will add it to exclusion list)
06:52:47.86 -06:19:16.7 -- not an asteroid (will add it to exclusion list)
06:45:33.70 -00:26:17.2 -- not an asteroid (will add it to exclusion list)
06:46:10.38 -03:13:58.6 -- not an asteroid (will add it to exclusion list)
06:47:23.66 +01:25:44.1 -- not an asteroid (will add it to exclusion list)
06:54:44.93 -01:17:25.8 -- not an asteroid (will add it to exclusion list)
07:05:25.58 -03:18:31.3 -- not an asteroid (will add it to exclusion list)
06:44:50.77 +01:05:45.2 -- not an asteroid (will add it to exclusion list)
07:11:11.59 -00:11:47.3 -- not an asteroid (will add it to exclusion list)
06:53:13.90 -04:35:48.3 -- not an asteroid (will add it to exclusion list)
07:09:21.64 +01:07:27.2 -- not an asteroid (will add it to exclusion list)
07:06:54.22 +02:10:49.2 -- not an asteroid (will add it to exclusion list)
06:45:17.67 +00:43:40.0 -- not an asteroid (will add it to exclusion list)
06:44:56.87 +01:18:45.6 -- not an asteroid (will add it to exclusion list)
07:14:23.48 -03:02:01.1 -- not an asteroid (will add it to exclusion list)
07:02:32.42 -00:13:09.4 -- not an asteroid (will add it to exclusion list)
06:38:07.57 +03:11:51.7 -- not an asteroid (will add it to exclusion list)
06:46:32.71 -01:51:13.3 -- not an asteroid (will add it to exclusion list)
06:47:59.60 -01:20:53.6 -- not an asteroid (will add it to exclusion list)
06:26:39.13 +00:26:39.7 -- not an asteroid (will add it to exclusion list)
06:59:49.89 -06:00:37.1 -- not an asteroid (will add it to exclusion list)
06:35:16.68 -01:19:06.8 -- not an asteroid (will add it to exclusion list)
06:46:18.39 -02:26:01.6 -- not an asteroid (will add it to exclusion list)
07:03:46.03 -02:09:32.8 -- not an asteroid (will add it to exclusion list)
07:03:07.01 +01:49:29.8 -- not an asteroid (will add it to exclusion list)
06:46:42.26 -05:47:35.3 -- not an asteroid (will add it to exclusion list)
07:07:03.77 -02:21:52.3 -- not an asteroid (will add it to exclusion list)
06:38:18.60 -03:21:23.7 -- not an asteroid (will add it to exclusion list)
06:44:12.58 -00:00:23.8 -- not an asteroid (will add it to exclusion list)
06:45:39.04 +02:45:22.7 -- not an asteroid (will add it to exclusion list)
06:47:20.31 +03:13:33.6 -- not an asteroid (will add it to exclusion list)
06:58:48.17 -00:36:47.5 -- not an asteroid (will add it to exclusion list)
06:59:10.77 -01:18:50.7 -- not an asteroid (will add it to exclusion list)
07:05:26.19 +01:29:35.0 -- not an asteroid (will add it to exclusion list)
07:04:19.80 +00:50:06.0 -- not an asteroid (will add it to exclusion list)
06:35:27.03 +00:29:41.6 -- not an asteroid (will add it to exclusion list)
07:17:24.01 +01:22:49.3 -- not an asteroid (will add it to exclusion list)
06:33:36.46 +02:19:22.9 -- not an asteroid (will add it to exclusion list)
07:05:42.94 -01:37:20.0 -- not an asteroid (will add it to exclusion list)
06:44:36.59 +00:59:55.7 -- not an asteroid (will add it to exclusion list)
06:51:01.05 +02:05:33.2 -- not an asteroid (will add it to exclusion list)
07:18:26.93 -01:08:11.3 -- not an asteroid (will add it to exclusion list)
06:53:47.35 -02:38:43.7 -- not an asteroid (will add it to exclusion list)
06:45:20.36 -01:12:37.2 -- not an asteroid (will add it to exclusion list)
06:48:04.88 +02:16:48.2 -- not an asteroid (will add it to exclusion list)
06:41:21.32 -00:35:22.9 -- not an asteroid (will add it to exclusion list)
06:44:38.19 -02:01:19.8 -- not an asteroid (will add it to exclusion list)
06:52:39.32 +00:08:53.5 -- not an asteroid (will add it to exclusion list)
06:21:05.81 -03:21:15.1 -- not an asteroid (will add it to exclusion list)
06:44:45.21 -04:22:27.7 -- not an asteroid (will add it to exclusion list)
06:54:49.15 -04:18:03.7 -- not an asteroid (will add it to exclusion list)
06:48:44.06 +02:01:36.7 -- not an asteroid (will add it to exclusion list)
06:46:12.27 +00:43:10.4 -- not an asteroid (will add it to exclusion list)
06:42:37.27 +02:58:09.2 -- not an asteroid (will add it to exclusion list)
07:21:14.34 +01:37:59.7 -- not an asteroid (will add it to exclusion list)
06:58:37.43 -06:48:35.7 -- not an asteroid (will add it to exclusion list)
07:13:18.55 -02:57:58.7 -- not an asteroid (will add it to exclusion list)
06:53:20.05 -00:02:21.4 -- not an asteroid (will add it to exclusion list)
06:43:24.84 -00:26:06.9 -- not an asteroid (will add it to exclusion list)
07:08:57.82 -01:26:26.5 -- not an asteroid (will add it to exclusion list)
06:39:16.36 -02:19:47.7 -- not an asteroid (will add it to exclusion list)
06:32:45.42 -00:27:20.1 -- not an asteroid (will add it to exclusion list)
07:08:53.85 +00:51:37.0 -- not an asteroid (will add it to exclusion list)
06:44:14.07 +02:30:45.5 -- not an asteroid (will add it to exclusion list)
06:58:34.51 -01:38:22.4 -- not an asteroid (will add it to exclusion list)
06:39:06.15 +00:32:10.0 -- not an asteroid (will add it to exclusion list)
07:02:45.57 -04:03:42.1 -- not an asteroid (will add it to exclusion list)
07:05:41.39 -03:03:49.3 -- not an asteroid (will add it to exclusion list)
06:46:55.19 +01:53:18.7 -- not an asteroid (will add it to exclusion list)
06:48:40.37 -01:40:11.7 -- not an asteroid (will add it to exclusion list)
07:00:46.17 +00:40:11.7 -- not an asteroid (will add it to exclusion list)
06:57:39.43 -03:34:42.5 -- not an asteroid (will add it to exclusion list)
06:54:27.95 -01:43:27.6 -- not an asteroid (will add it to exclusion list)
07:05:08.88 -03:40:22.2 -- not an asteroid (will add it to exclusion list)
07:12:27.96 -04:46:31.0 -- not an asteroid (will add it to exclusion list)
06:39:31.84 -01:20:52.1 -- not an asteroid (will add it to exclusion list)
06:51:24.01 +02:19:39.4 -- not an asteroid (will add it to exclusion list)
06:38:16.13 -00:57:51.9 -- not an asteroid (will add it to exclusion list)
06:44:44.47 +03:07:31.7 -- not an asteroid (will add it to exclusion list)
07:09:13.70 -02:21:30.6 -- not an asteroid (will add it to exclusion list)
07:17:31.29 +01:05:39.2 -- not an asteroid (will add it to exclusion list)
07:12:42.41 -04:32:29.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:21:05.81 -03:21:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:39.13 +00:26:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:32.93 -02:51:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:03.44 +01:18:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:15.28 +02:16:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:45.42 -00:27:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:18.02 +00:28:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:36.46 +02:19:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:11.12 -00:21:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:10.43 -00:43:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:16.68 -01:19:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:21.92 -05:17:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:27.03 +00:29:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:32.34 -03:35:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:46.77 +02:28:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:07.57 +03:11:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:16.13 -00:57:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:18.60 -03:21:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:06.15 +00:32:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:16.36 -02:19:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:20.08 +00:23:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:31.84 -01:20:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:41.67 +01:09:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:53.99 +02:23:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.49 -01:04:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.32 -00:35:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.76 +02:47:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:43.54 -01:05:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:58.52 +02:45:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:00.96 +00:23:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.27 -03:28:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:37.27 +02:58:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:24.84 -00:26:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:27.95 -03:56:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:32.68 +01:24:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:39.43 +03:05:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:42.50 -04:26:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:50.85 +01:35:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:51.27 +03:09:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:12.58 -00:00:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:14.07 +02:30:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:16.61 -00:10:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.59 +00:59:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:38.19 -02:01:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:44.47 +03:07:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:45.21 -04:22:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.77 +01:05:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:56.87 +01:18:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:05.03 +02:42:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.67 +00:43:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:20.36 -01:12:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.70 -00:26:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:34.10 +03:08:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.04 +02:45:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.38 -03:13:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:12.27 +00:43:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:18.39 -02:26:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.57 -00:28:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.71 -01:51:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:42.26 -05:47:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:55.19 +01:53:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:56.75 +01:41:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:20.31 +03:13:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:23.66 +01:25:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.60 -01:20:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:04.88 +02:16:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:07.75 -00:40:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.43 -05:22:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.54 +01:46:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:38.13 +02:54:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:40.37 -01:40:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:44.06 +02:01:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:26.79 +02:25:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.77 -03:29:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:45.36 +01:03:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:49.69 -01:13:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.53 +00:13:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:01.05 +02:05:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:24.01 +02:19:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:40.94 -00:36:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.51 -01:18:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:39.32 +00:08:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:47.86 -06:19:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:13.90 -04:35:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:20.05 -00:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.35 -02:38:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:50.85 -00:03:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:27.95 -01:43:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.44 +02:38:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:44.93 -01:17:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:49.15 -04:18:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.23 -01:02:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:39.03 -06:15:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:04.45 -01:29:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:14.69 -03:49:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:30.70 +01:10:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:36.62 +02:42:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.36 -03:57:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:22.85 +02:20:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:24.16 -00:50:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:38.25 +02:11:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:39.43 -03:34:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.70 -01:31:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:08.39 -01:38:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.51 -01:38:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:37.43 -06:48:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:48.17 -00:36:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:10.77 -01:18:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:35.47 +00:38:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:38.82 -01:27:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:49.89 -06:00:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:39.12 -01:30:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:46.17 +00:40:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:12.34 -00:55:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.59 +00:57:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:16.10 -02:29:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:36.99 -04:32:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:02.05 -01:53:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:08.18 +02:42:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.69 -01:34:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.42 -00:13:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:33.63 -01:57:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:45.57 -04:03:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:53.01 -04:59:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.49 -01:18:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:06.49 -05:17:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:07.01 +01:49:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.88 +02:37:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:46.03 -02:09:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:05.58 +00:58:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.78 -03:01:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:19.80 +00:50:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:32.09 +00:11:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.61 -02:12:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:54.61 +00:11:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:08.88 -03:40:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:12.17 -03:19:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:13.23 -06:04:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:25.58 -03:18:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:26.19 +01:29:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.39 -03:03:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:42.94 -01:37:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:57.75 +02:49:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.95 +00:18:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.75 +01:08:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.22 +02:10:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:03.77 -02:21:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:04.86 -03:10:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:07.01 +01:40:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:33.42 -03:25:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:40.41 -03:15:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:13.33 -04:47:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:17.17 -04:56:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:24.33 -01:19:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:25.19 +02:46:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.63 +01:46:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.53 +01:59:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.88 +01:25:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:53.85 +00:51:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:57.82 -01:26:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.70 -02:21:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.65 +02:38:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.64 +01:07:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:29.04 -06:44:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:57.35 -01:59:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.13 -00:55:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:14.40 -00:48:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:18.71 -01:17:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:55.07 -00:54:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:55.84 -00:46:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:11.59 -00:11:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:30.24 +00:31:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:37.57 -06:35:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:55.44 -04:52:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:11.47 -02:24:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:27.96 -04:46:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:29.44 -01:56:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:39.26 -06:53:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:42.41 -04:32:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:18.55 -02:57:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:32.81 +00:13:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:02.19 -01:05:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:23.48 -03:02:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:07.29 +02:40:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:10.17 +00:22:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:26.09 -01:11:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:00.07 +01:17:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:04.08 +02:09:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:09.62 +02:29:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:24.01 +01:22:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.29 +01:05:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.42 -00:53:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:50.85 -01:41:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:22.69 +00:37:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:26.93 -01:08:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:31.83 -06:47:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:48.76 -01:43:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:08.24 -02:01:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:23.98 -02:42:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:37.64 -02:20:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:22.44 +01:19:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:34.18 -00:45:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:41.13 -03:34:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:48.34 -06:16:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:50.33 -00:51:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:06.36 -03:15:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:12.24 -01:21:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:14.34 +01:37:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:26.66 -03:34:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:21:05.81 -03:21:15.1 -- not a known variable star
06:26:39.13 +00:26:39.7 -- not a known variable star
06:29:32.93 -02:51:13.6 -- not a known variable star
06:30:03.44 +01:18:36.1 -- a known variable star
06:30:15.28 +02:16:00.3 -- not a known variable star
06:32:45.42 -00:27:20.1 -- not a known variable star
06:33:18.02 +00:28:22.1 -- not a known variable star
06:33:36.46 +02:19:22.9 -- not a known variable star
06:34:11.12 -00:21:48.8 -- not a known variable star
06:35:10.43 -00:43:20.3 -- not a known variable star
06:35:16.68 -01:19:06.8 -- a known variable star
06:35:21.92 -05:17:33.0 -- not a known variable star
06:35:27.03 +00:29:41.6 -- not a known variable star
06:36:32.34 -03:35:55.8 -- not a known variable star
06:36:46.77 +02:28:24.3 -- not a known variable star
06:38:07.57 +03:11:51.7 -- not a known variable star
06:38:16.13 -00:57:51.9 -- not a known variable star
06:38:18.60 -03:21:23.7 -- not a known variable star
06:39:06.15 +00:32:10.0 -- not a known variable star
06:39:16.36 -02:19:47.7 -- a known variable star
06:39:20.08 +00:23:03.7 -- a known variable star
06:39:31.84 -01:20:52.1 -- not a known variable star
06:39:41.67 +01:09:51.9 -- not a known variable star
06:39:53.99 +02:23:22.4 -- not a known variable star
06:40:30.49 -01:04:41.9 -- a known variable star
06:41:21.32 -00:35:22.9 -- not a known variable star
06:41:26.76 +02:47:59.5 -- not a known variable star
06:41:43.54 -01:05:57.1 -- not a known variable star
06:41:58.52 +02:45:41.4 -- not a known variable star
06:42:00.96 +00:23:10.9 -- not a known variable star
06:42:33.27 -03:28:04.5 -- not a known variable star
06:42:37.27 +02:58:09.2 -- not a known variable star
06:43:24.84 -00:26:06.9 -- not a known variable star
06:43:27.95 -03:56:28.9 -- a known variable star
06:43:32.68 +01:24:31.8 -- not a known variable star
06:43:39.43 +03:05:01.9 -- not a known variable star
06:43:42.50 -04:26:30.0 -- a known variable star
06:43:50.85 +01:35:53.8 -- not a known variable star
06:43:51.27 +03:09:10.1 -- not a known variable star
06:44:12.58 -00:00:23.8 -- not a known variable star
06:44:14.07 +02:30:45.5 -- not a known variable star
06:44:16.61 -00:10:05.4 -- not a known variable star
06:44:36.59 +00:59:55.7 -- not a known variable star
06:44:38.19 -02:01:19.8 -- not a known variable star
06:44:44.47 +03:07:31.7 -- not a known variable star
06:44:45.21 -04:22:27.7 -- not a known variable star
06:44:50.77 +01:05:45.2 -- not a known variable star
06:44:56.87 +01:18:45.6 -- not a known variable star
06:45:05.03 +02:42:58.0 -- not a known variable star
06:45:17.67 +00:43:40.0 -- not a known variable star
06:45:20.36 -01:12:37.2 -- not a known variable star
06:45:33.70 -00:26:17.2 -- a known variable star
06:45:34.10 +03:08:05.6 -- not a known variable star
06:45:39.04 +02:45:22.7 -- a known variable star
06:46:10.38 -03:13:58.6 -- a known variable star
06:46:12.27 +00:43:10.4 -- not a known variable star
06:46:18.39 -02:26:01.6 -- a known variable star
06:46:25.57 -00:28:35.9 -- not a known variable star
06:46:32.71 -01:51:13.3 -- not a known variable star
06:46:42.26 -05:47:35.3 -- not a known variable star
06:46:55.19 +01:53:18.7 -- not a known variable star
06:46:56.75 +01:41:48.2 -- not a known variable star
06:47:20.31 +03:13:33.6 -- not a known variable star
06:47:23.66 +01:25:44.1 -- a known variable star
06:47:59.60 -01:20:53.6 -- not a known variable star
06:48:04.88 +02:16:48.2 -- a known variable star
06:48:07.75 -00:40:38.3 -- not a known variable star
06:48:15.43 -05:22:39.6 -- not a known variable star
06:48:15.54 +01:46:16.6 -- not a known variable star
06:48:38.13 +02:54:38.4 -- not a known variable star
06:48:40.37 -01:40:11.7 -- a known variable star
06:48:44.06 +02:01:36.7 -- not a known variable star
06:49:26.79 +02:25:16.6 -- not a known variable star
06:50:09.77 -03:29:01.2 -- a known variable star
06:50:45.36 +01:03:08.2 -- not a known variable star
06:50:49.69 -01:13:39.2 -- not a known variable star
06:50:59.53 +00:13:39.9 -- not a known variable star
06:51:01.05 +02:05:33.2 -- a known variable star
06:51:24.01 +02:19:39.4 -- a known variable star
06:51:40.94 -00:36:47.3 -- a known variable star
06:52:06.51 -01:18:21.8 -- not a known variable star
06:52:39.32 +00:08:53.5 -- a known variable star
06:52:47.86 -06:19:16.7 -- not a known variable star
06:53:13.90 -04:35:48.3 -- not a known variable star
06:53:20.05 -00:02:21.4 -- not a known variable star
06:53:47.35 -02:38:43.7 -- not a known variable star
06:53:50.85 -00:03:50.8 -- not a known variable star
06:54:27.95 -01:43:27.6 -- not a known variable star
06:54:39.44 +02:38:01.5 -- not a known variable star
06:54:44.93 -01:17:25.8 -- not a known variable star
06:54:49.15 -04:18:03.7 -- not a known variable star
06:55:03.23 -01:02:51.0 -- not a known variable star
06:55:39.03 -06:15:20.8 -- not a known variable star
06:56:04.45 -01:29:59.6 -- not a known variable star
06:56:14.69 -03:49:56.7 -- not a known variable star
06:56:30.70 +01:10:47.6 -- not a known variable star
06:56:36.62 +02:42:44.9 -- not a known variable star
06:57:12.36 -03:57:42.9 -- not a known variable star
06:57:22.85 +02:20:23.7 -- not a known variable star
06:57:24.16 -00:50:14.3 -- not a known variable star
06:57:38.25 +02:11:06.7 -- not a known variable star
06:57:39.43 -03:34:42.5 -- not a known variable star
06:57:47.70 -01:31:07.3 -- a known variable star
06:58:08.39 -01:38:49.8 -- not a known variable star
06:58:34.51 -01:38:22.4 -- not a known variable star
06:58:37.43 -06:48:35.7 -- not a known variable star
06:58:48.17 -00:36:47.5 -- not a known variable star
06:59:10.77 -01:18:50.7 -- not a known variable star
06:59:35.47 +00:38:55.5 -- a known variable star
06:59:38.82 -01:27:09.2 -- a known variable star
06:59:49.89 -06:00:37.1 -- not a known variable star
07:00:39.12 -01:30:26.1 -- not a known variable star
07:00:46.17 +00:40:11.7 -- not a known variable star
07:01:12.34 -00:55:21.7 -- a known variable star
07:01:14.59 +00:57:29.3 -- not a known variable star
07:01:16.10 -02:29:02.8 -- not a known variable star
07:01:36.99 -04:32:42.3 -- not a known variable star
07:02:02.05 -01:53:45.0 -- a known variable star
07:02:08.18 +02:42:03.7 -- not a known variable star
07:02:23.69 -01:34:41.1 -- not a known variable star
07:02:32.42 -00:13:09.4 -- not a known variable star
07:02:33.63 -01:57:58.4 -- not a known variable star
07:02:45.57 -04:03:42.1 -- not a known variable star
07:02:53.01 -04:59:09.0 -- not a known variable star
07:03:04.49 -01:18:37.3 -- not a known variable star
07:03:06.49 -05:17:29.6 -- not a known variable star
07:03:07.01 +01:49:29.8 -- a known variable star
07:03:36.88 +02:37:11.3 -- a known variable star
07:03:46.03 -02:09:32.8 -- not a known variable star
07:04:05.58 +00:58:05.8 -- not a known variable star
07:04:16.78 -03:01:36.9 -- not a known variable star
07:04:19.80 +00:50:06.0 -- not a known variable star
07:04:32.09 +00:11:21.8 -- a known variable star
07:04:51.61 -02:12:04.2 -- not a known variable star
07:04:54.61 +00:11:37.3 -- not a known variable star
07:05:08.88 -03:40:22.2 -- not a known variable star
07:05:12.17 -03:19:36.5 -- not a known variable star
07:05:13.23 -06:04:45.2 -- not a known variable star
07:05:25.58 -03:18:31.3 -- not a known variable star
07:05:26.19 +01:29:35.0 -- a known variable star
07:05:41.39 -03:03:49.3 -- not a known variable star
07:05:42.94 -01:37:20.0 -- not a known variable star
07:05:57.75 +02:49:17.9 -- not a known variable star
07:06:11.95 +00:18:35.4 -- not a known variable star
07:06:31.75 +01:08:40.3 -- a known variable star
07:06:54.22 +02:10:49.2 -- a known variable star
07:07:03.77 -02:21:52.3 -- not a known variable star
07:07:04.86 -03:10:06.2 -- not a known variable star
07:07:07.01 +01:40:01.5 -- not a known variable star
07:07:33.42 -03:25:31.7 -- a known variable star
07:07:40.41 -03:15:05.7 -- a known variable star
07:08:13.33 -04:47:30.8 -- not a known variable star
07:08:17.17 -04:56:00.9 -- a known variable star
07:08:24.33 -01:19:54.2 -- not a known variable star
07:08:25.19 +02:46:17.6 -- not a known variable star
07:08:35.63 +01:46:44.6 -- not a known variable star
07:08:43.53 +01:59:22.8 -- not a known variable star
07:08:45.88 +01:25:42.4 -- not a known variable star
07:08:53.85 +00:51:37.0 -- not a known variable star
07:08:57.82 -01:26:26.5 -- not a known variable star
07:09:13.70 -02:21:30.6 -- a known variable star
07:09:20.65 +02:38:45.3 -- not a known variable star
07:09:21.64 +01:07:27.2 -- a known variable star
07:09:29.04 -06:44:33.8 -- not a known variable star
07:09:57.35 -01:59:05.9 -- not a known variable star
07:10:10.13 -00:55:10.3 -- not a known variable star
07:10:14.40 -00:48:25.3 -- not a known variable star
07:10:18.71 -01:17:10.7 -- not a known variable star
07:10:55.07 -00:54:14.1 -- a known variable star
07:10:55.84 -00:46:11.3 -- a known variable star
07:11:11.59 -00:11:47.3 -- a known variable star
07:11:30.24 +00:31:17.4 -- not a known variable star
07:11:37.57 -06:35:51.4 -- not a known variable star
07:11:55.44 -04:52:52.9 -- a known variable star
07:12:11.47 -02:24:18.3 -- not a known variable star
07:12:27.96 -04:46:31.0 -- not a known variable star
07:12:29.44 -01:56:23.7 -- not a known variable star
07:12:39.26 -06:53:46.5 -- not a known variable star
07:12:42.41 -04:32:29.3 -- a known variable star
07:13:18.55 -02:57:58.7 -- a known variable star
07:13:32.81 +00:13:14.5 -- a known variable star
07:14:02.19 -01:05:33.3 -- not a known variable star
07:14:23.48 -03:02:01.1 -- not a known variable star
07:15:07.29 +02:40:51.9 -- not a known variable star
07:15:10.17 +00:22:00.4 -- not a known variable star
07:15:26.09 -01:11:22.2 -- not a known variable star
07:16:00.07 +01:17:46.5 -- not a known variable star
07:16:04.08 +02:09:50.7 -- not a known variable star
07:17:09.62 +02:29:28.1 -- not a known variable star
07:17:24.01 +01:22:49.3 -- not a known variable star
07:17:31.29 +01:05:39.2 -- a known variable star
07:17:31.42 -00:53:39.9 -- a known variable star
07:17:50.85 -01:41:24.3 -- a known variable star
07:18:22.69 +00:37:20.2 -- a known variable star
07:18:26.93 -01:08:11.3 -- not a known variable star
07:18:31.83 -06:47:04.5 -- a known variable star
07:18:48.76 -01:43:49.2 -- not a known variable star
07:19:08.24 -02:01:49.4 -- not a known variable star
07:19:23.98 -02:42:21.2 -- not a known variable star
07:19:37.64 -02:20:15.6 -- not a known variable star
07:20:22.44 +01:19:55.4 -- not a known variable star
07:20:34.18 -00:45:32.6 -- not a known variable star
07:20:41.13 -03:34:37.7 -- not a known variable star
07:20:48.34 -06:16:18.5 -- not a known variable star
07:20:50.33 -00:51:22.7 -- a known variable star
07:21:06.36 -03:15:03.6 -- not a known variable star
07:21:12.24 -01:21:16.4 -- a known variable star
07:21:14.34 +01:37:59.7 -- not a known variable star
07:21:26.66 -03:34:46.4 -- not a known variable star
Found 160 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
209 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 209 (excluding asteroids and hot pixels, 160 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)2461148.61673056 -observatory V36
00:18:41.01 -00:50:55.4 Mercury (-0.0mag)
03:19:02.25 +18:38:00.9 Venus (-3.9mag)
00:23:50.94 +01:31:30.7 Mars (1.2mag)
07:13:36.99 +22:44:36.1 Jupiter (-2.1mag)
00:30:07.24 +00:54:49.7 Saturn (0.9mag)
03:48:08.80 +19:48:54.9 Uranus (5.8mag)
00:11:06.91 -00:13:38.5 Neptune (7.8mag)
20:33:50.55 -22:52:42.7 Pluto (14.5mag)
02:06:37.70 +17:08:16.7 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 Apr 17 21:53 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461148.61673056:
07:13:43.60 +22:44:23.6 Io (5.8mag)
07:13:28.26 +22:44:52.8 Europa (5.9mag)
07:13:23.83 +22:44:58.3 Ganymede (5.4mag)
07:14:03.42 +22:43:35.0 Callisto (6.6mag)
07:16:51.50 +22:31:15.8 Himalia (15.3mag)
07:13:36.13 +22:44:35.7 Thebe (16.2mag)
07:17:05.53 +23:01:33.9 Elara (17.3mag)
07:12:38.51 +23:23:30.0 Pasiphae (17.4mag)
07:21:53.81 +22:42:49.5 Carme (18.5mag)
00:30:00.52 +00:55:16.1 Titan (8.8mag)
00:30:12.34 +00:54:57.3 Rhea (10.1mag)
00:29:43.92 +00:54:38.7 Iapetus (11.5mag)
00:30:07.38 +00:55:17.1 Hyperion (14.8mag)
00:31:42.43 +01:03:24.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 17 21:53 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461148.61673056:
15:47:30.10 -17:40:45.5 JWST
19:14:35.54 +13:24:21.9 Chandra
07:52:19.09 -34:28:37.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 17 21:53 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461148.61673056 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:48.85 -28:54:18.0 13.9mag P/2010 H2 (Vales)
05:08:16.57 -69:33:47.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:55.03 +31:27:07.8 17.2mag C/2017 K2 (PANSTARRS)
17:30:12.10 +10:47:48.5 17.6mag C/2021 G2 (ATLAS)
23:10:46.09 +29:18:51.3 17.1mag C/2022 E2 (ATLAS)
04:31:42.79 +26:05:42.9 16.0mag C/2022 N2 (PANSTARRS)
09:03:54.52 +32:01:37.5 16.2mag C/2022 QE78 (ATLAS)
08:31:25.48 +00:04:04.9 17.3mag C/2022 R6 (PANSTARRS)
18:53:12.01 +18:42:31.2 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:58.19 -11:29:25.6 17.5mag P/2023 B1 (PANSTARRS)
09:06:41.83 -11:32:52.6 17.7mag C/2023 F3 (ATLAS)
21:56:16.86 +63:01:57.3 17.5mag C/2023 H5 (Lemmon)
19:17:17.13 -03:46:12.6 14.1mag C/2023 R1 (PANSTARRS)
21:27:27.60 +86:12:25.7 17.8mag C/2023 X2 (Lemmon)
06:18:57.22 +63:30:20.3 17.2mag C/2024 A1 (ATLAS)
05:17:45.38 +18:59:14.9 11.2mag C/2024 E1 (Wierzchos)
16:17:53.23 +06:44:10.8 17.4mag C/2024 G6 (ATLAS)
20:21:22.13 +15:51:13.4 14.6mag C/2024 J3 (ATLAS)
03:28:16.86 -22:03:59.3 16.3mag C/2024 T5 (ATLAS)
05:18:31.50 +44:46:20.5 17.7mag C/2025 J1 (Borisov)
13:30:05.79 +46:46:34.8 15.3mag C/2025 L1 (ATLAS)
03:28:39.56 -26:32:49.9 17.8mag C/2025 Q3 (ATLAS)
00:05:09.24 +17:39:53.9 8.2mag C/2025 R3 (PANSTARRS)
12:53:12.47 +03:08:21.3 17.4mag C/2025 Y1 (ATLAS)
03:44:07.26 +02:25:04.6 13.9mag C/2026 A1 (MAPS)
00:05:31.22 +37:35:56.8 14.6mag C/2026 B2 (Sun-Gao)
18:47:03.05 -09:36:16.3 11.7mag 10P/Tempel
14:57:25.53 +02:58:51.9 14.2mag 24P/Schaumasse
11:02:15.68 -01:27:34.6 15.7mag 29P/Schwassmann-Wachmann
18:01:29.11 -09:32:03.8 18.0mag 40P/Vaisala
10:37:32.35 -03:56:10.0 16.9mag 43P/Wolf-Harrington
01:51:57.21 +17:50:48.5 17.2mag 47P/Ashbrook-Jackson
07:14:42.70 +36:33:18.6 17.0mag 63P/Wild
23:31:44.31 -11:11:55.2 15.7mag 65P/Gunn
04:08:56.90 +21:58:19.3 15.9mag 76P/West-Kohoutek-Ikemura
01:10:16.06 +08:38:35.0 14.3mag 78P/Gehrels
23:09:21.67 -08:45:53.1 14.6mag 88P/Howell
02:16:25.61 +21:12:01.0 15.1mag 93P/Lovas
04:58:50.04 +32:23:52.2 16.2mag 123P/West-Hartley
08:30:55.28 +37:23:08.3 16.2mag 124P/Mrkos
02:36:29.86 +14:36:16.3 16.4mag 128P/Shoemaker-Holt
02:51:41.83 +14:44:53.3 17.5mag 131P/Mueller
01:37:21.46 +13:56:58.9 10.6mag 141P/Machholz
01:45:58.19 +05:39:53.9 10.6mag 141P-A/Machholz
00:30:17.81 +01:30:23.5 12.6mag 141P-D/Machholz
02:16:26.66 +07:25:25.1 17.8mag 141P-I/Machholz
01:08:17.61 -00:27:31.5 15.0mag 162P/SidingSpring
14:47:41.12 +00:08:27.4 17.7mag 210P/Christensen
21:44:52.03 -10:56:25.2 17.7mag 218P/LINEAR
17:16:59.98 -13:40:36.1 16.1mag 235P/LINEAR
05:39:04.63 +34:51:09.2 16.8mag 240P/NEAT
07:39:34.14 -04:56:32.1 17.7mag 242P/Spahr
22:22:12.08 -20:24:29.0 17.8mag 260P/McNaught
02:02:31.97 +20:59:27.3 18.0mag 295P/LINEAR
15:41:47.43 +07:07:37.0 17.5mag 391P/Kowalski
07:35:02.46 +21:22:15.5 17.7mag 450P/LONEOS
05:38:58.89 +44:54:32.7 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 17 21:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
-rw-r--r-- 1 apache apache 5.8K Apr 17 21:53 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 17 21:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:52:44.230 +56:55:19.06 AT 2026jfc 2026-03-27.87 20.98
14:01:07.200 +03:10:48.03 AT 2026jfb 2026-04-05.73 21.73
13:47:01.080 +02:47:45.39 AT 2026jfa 2026-03-24.91 20.68
17:11:20.724 -17:18:29.68 AT 2026jez 2026-04-04.38 17.507
03:59:36.404 -57:03:28.57 AT 2026jey 2026-04-05.01 18.79
03:57:56.301 -54:05:57.45 AT 2026jex 2026-04-08.01 19.148
10:30:49.649 -08:04:36.38 AT 2026jew 2026-04-07.87 19.144
12:27:21.393 -28:22:09.12 AT 2026jev 2026-04-10.19 18.809
17:40:25.287 +05:08:20.96 AT 2026jeu 2026-04-05.42 17.65
08:35:16.434 -77:00:48.01 AT 2026jet 2026-04-09.11 19.072
21:53:03.051 -16:55:33.84 AT 2026jes 2026-04-10.38 17.345
00:36:19.401 -83:06:05.82 AT 2026jer 2026-04-08.40 18.473
22:08:10.236 -21:46:23.75 AT 2026jeq 2026-04-10.39 18.259
21:34:17.331 -33:37:48.49 AT 2026jep 2026-04-10.39 18.372
16:56:26.248 +04:54:42.94 AT 2026jeo 2026-04-10.42 18.3645
08:10:18.680 +34:40:45.43 AT 2026jen 2026-04-05.17 20.6002
10:14:46.220 +16:03:20.00 AT 2026jem 2026-04-07.20 20.5179
09:08:33.148 +56:28:29.17 AT 2026jel 2026-04-09.15 19.5877
08:06:59.814 +72:49:07.23 AT 2026jek 2026-04-05.15 20.127
10:17:15.279 +45:17:14.78 AT 2026jej 2026-04-08.19 20.2002
-rw-r--r-- 1 apache apache 30K Apr 17 21:53 tns_transients_list.txt
