This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg
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
ATO J102.8479+00.5677,2461146.6091,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8479+00.5677 20260416.1091 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112515039375055744,2461146.6091,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112515039375055744 20260416.1091 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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 3102159430849022592,2461146.6091,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102159430849022592 20260416.1091 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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 3101124137571642112,2461146.6091,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101124137571642112 20260416.1091 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106277789090410496,2461146.6091,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106277789090410496 20260416.1091 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 J101.5794-01.9625,2461146.6091,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.5794-01.9625 20260416.1091 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
ASAS J064451-0451.4,2461146.6091,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J064451-0451.4 20260416.1091 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119846071812024192,2461146.6091,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119846071812024192 20260416.1091 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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 J104.2008-01.0734,2461146.6091,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2008-01.0734 20260416.1091 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.0781-01.8195,2461146.6091,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.0781-01.8195 20260416.1091 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3015+00.9263,2461146.6091,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3015+00.9263 20260416.1091 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4280-01.9828,2461146.6091,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4280-01.9828 20260416.1091 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112536277993759872,2461146.6091,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112536277993759872 20260416.1091 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112222539223581184,2461146.6091,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112222539223581184 20260416.1091 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100432819636957184,2461146.6091,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100432819636957184 20260416.1091 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064630.95+010809.2,2461146.6091,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064630.95+010809.2 20260416.1091 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 3106045203719510272,2461146.6091,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106045203719510272 20260416.1091 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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 3112321495271112192,2461146.6091,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112321495271112192 20260416.1091 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113790030488561920,2461146.6091,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113790030488561920 20260416.1091 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 3107406673992729472,2461146.6091,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107406673992729472 20260416.1091 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7849-02.6590,2461146.6091,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7849-02.6590 20260416.1091 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
target,2461146.6091,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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
target,2461146.6091,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.1971+01.7168,2461146.6091,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.1971+01.7168 20260416.1091 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 3105965733946504448,2461146.6091,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105965733946504448 20260416.1091 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 3105924742777831040,2461146.6091,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105924742777831040 20260416.1091 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
target,2461146.6091,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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
ATO J098.7797-03.0546,2461146.6091,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260416.1091 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8560-01.8007,2461146.6091,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8560-01.8007 20260416.1091 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 3113286419803767168,2461146.6091,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113286419803767168 20260416.1091 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107032775621691520,2461146.6091,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107032775621691520 20260416.1091 12.17CV 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
NSVS 12569794,2461146.6091,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12569794 20260416.1091 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113311193174967552,2461146.6091,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113311193174967552 20260416.1091 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065134.58+002720.2,2461146.6091,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065134.58+002720.2 20260416.1091 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3075-00.0345,2461146.6091,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3075-00.0345 20260416.1091 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113144097467624576,2461146.6091,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113144097467624576 20260416.1091 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065448.56+002321.1,2461146.6091,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065448.56+002321.1 20260416.1091 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6619-02.2718,2461146.6091,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6619-02.2718 20260416.1091 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4869-02.9025,2461146.6091,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.4869-02.9025 20260416.1091 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 J103.2327-02.3822,2461146.6091,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2327-02.3822 20260416.1091 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6947-02.6960,2461146.6091,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6947-02.6960 20260416.1091 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112314039208032000,2461146.6091,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112314039208032000 20260416.1091 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 J100.6477-03.4721,2461146.6091,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6477-03.4721 20260416.1091 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 3112121349793909632,2461146.6091,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112121349793909632 20260416.1091 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107281540128223104,2461146.6091,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107281540128223104 20260416.1091 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105947282767695360,2461146.6091,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105947282767695360 20260416.1091 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
MGAB-V1900,2461146.6091,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MGAB-V1900 20260416.1091 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 J102.9043-01.6544,2461146.6091,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9043-01.6544 20260416.1091 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5787+00.4180,2461146.6091,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5787+00.4180 20260416.1091 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 3106035656015561472,2461146.6091,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106035656015561472 20260416.1091 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,2461146.6091,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106128697885405184,2461146.6091,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106128697885405184 20260416.1091 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 3100477590376004224,2461146.6091,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100477590376004224 20260416.1091 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 3104844811903742208,2461146.6091,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3104844811903742208 20260416.1091 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9776-05.0786,2461146.6091,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9776-05.0786 20260416.1091 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 3112503842401083904,2461146.6091,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112503842401083904 20260416.1091 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 3100639940141069696,2461146.6091,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100639940141069696 20260416.1091 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 3113913996125565440,2461146.6091,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260416.1091 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 3113219246514568576,2461146.6091,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260416.1091 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113470691079092224,2461146.6091,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113470691079092224 20260416.1091 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113525082544566656,2461146.6091,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113525082544566656 20260416.1091 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106831938650976384,2461146.6091,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106831938650976384 20260416.1091 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7529-00.5089,2461146.6091,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.7529-00.5089 20260416.1091 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302831513609216,2461146.6091,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105302831513609216 20260416.1091 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113647334495911936,2461146.6091,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113647334495911936 20260416.1091 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 3125607134785759744,2461146.6091,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125607134785759744 20260416.1091 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 3100441267835993600,2461146.6091,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100441267835993600 20260416.1091 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 3105494249614626944,2461146.6091,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105494249614626944 20260416.1091 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 3113700076693885568,2461146.6091,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113700076693885568 20260416.1091 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5128+02.1105,2461146.6091,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.5128+02.1105 20260416.1091 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 3113580985840495488,2461146.6091,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113580985840495488 20260416.1091 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4491-02.6658,2461146.6091,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4491-02.6658 20260416.1091 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3335+01.2242,2461146.6091,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.3335+01.2242 20260416.1091 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 J101.6375-01.8671,2461146.6091,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.6375-01.8671 20260416.1091 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1615-02.0240,2461146.6091,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1615-02.0240 20260416.1091 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 3119355071151771648,2461146.6091,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119355071151771648 20260416.1091 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 3113408362514158720,2461146.6091,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113408362514158720 20260416.1091 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TY Mon,2461146.6091,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TY Mon 20260416.1091 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 3102364077450053120,2461146.6091,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102364077450053120 20260416.1091 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106070840385622144,2461146.6091,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106070840385622144 20260416.1091 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7913+00.9506,2461146.6091,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7913+00.9506 20260416.1091 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103722455347900032,2461146.6091,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103722455347900032 20260416.1091 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 J103.9614-02.2114,2461146.6091,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9614-02.2114 20260416.1091 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
ATO J101.5488+00.7303,2461146.6091,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.5488+00.7303 20260416.1091 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112396051604609408,2461146.6091,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112396051604609408 20260416.1091 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 J101.3361+01.6249,2461146.6091,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3361+01.6249 20260416.1091 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106335719608696832,2461146.6091,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106335719608696832 20260416.1091 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3694-00.1977,2461146.6091,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3694-00.1977 20260416.1091 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126343429620148736,2461146.6091,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126343429620148736 20260416.1091 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 J103.8575+00.6544,2461146.6091,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8575+00.6544 20260416.1091 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0736-03.3663,2461146.6091,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0736-03.3663 20260416.1091 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102395001214275712,2461146.6091,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102395001214275712 20260416.1091 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2470-00.3976,2461146.6091,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2470-00.3976 20260416.1091 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 3105706794657490816,2461146.6091,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105706794657490816 20260416.1091 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 J100.7244-04.5103,2461146.6091,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.7244-04.5103 20260416.1091 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2554+01.4334,2461146.6091,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2554+01.4334 20260416.1091 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 3112353243668770304,2461146.6091,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112353243668770304 20260416.1091 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106335238572484096,2461146.6091,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106335238572484096 20260416.1091 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9492-01.1270,2461146.6091,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9492-01.1270 20260416.1091 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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,2461146.6091,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.86CV 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 3113763912787484672,2461146.6091,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113763912787484672 20260416.1091 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 3113126131624754560,2461146.6091,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113126131624754560 20260416.1091 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6091,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1091 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
Date (UTC)
JD(UTC)
mag.
R.A. & Dec.(J2000)
X & Y (pix)
Image
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0276-01.3052,2461146.6091,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0276-01.3052 20260416.1091 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461146.60940014 16.04.2026 02:37:22.172 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.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: 7 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): 32233
Objects passed selection criteria: 32111
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 25921
Average stars matched: 23359 (90.1161 %)
Memory usage VmPeak: 132412 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:11:40 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461146.60940014 16.04.2026 02:37:22.172 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 563
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 298 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): 235334
Objects passed selection criteria: 234502
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 192528
Average stars matched: 173832 (90.2887 %)
Memory usage VmPeak: 1986716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:18:17 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.60882257
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
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
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Image size: 925.0'x622.6' 15.4(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 06:51:30.811 -01:59:12.56 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 06:51:30.811 -01:59:12.56
Angular distance between the image centers 0.0541 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:32.084 -01:59:53.91 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 06:51:32.084 -01:59:53.91
Angular distance between the image centers 0.0462 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 06:51:30.811 -01:59:12.56
Second-epoch second image center 06:51:32.084 -01:59:53.91
Angular distance between the image centers 0.01265 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.GEbssMb1co
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.fyKhtESCIH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits &> /tmp/tmp.BWvbf7Pvzz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits &> /tmp/tmp.7zXVWo3ED2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.8 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
14.8 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GEbssMb1co (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fyKhtESCIH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BWvbf7Pvzz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3302, passed=30556
Got 30556 stars (including 27232 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 30556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 925.0'
Seting catalog search parameters based on the expected field of view 925.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012847 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010278 (37.0 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 670 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 612 matched stars entering correct_measured_positions(), 557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.01"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 610 matched stars entering correct_measured_positions(), 15327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.41"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 711 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 660 matched stars entering correct_measured_positions(), 15346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.35"
Accuracy estimation diagnostic: 659 matched stars entering correct_measured_positions(), 16308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.00"
Excluding outliers - 659 stars left (next iteration limit 671)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.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.7zXVWo3ED2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3253, passed=30606
Got 30606 stars (including 27331 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 30606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 30094 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 30093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 30094 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58412.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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
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Considering the candidate 51880_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 51880_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 51884_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 51884_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (211.4") between the two second-epoch detections
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Considering the candidate 51885_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 51885_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:07.54 -01:28:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.00, MAG_FAINT_SEARCH_LIMIT=11.98)GAIADR2_OUTPUT=# 1.549 3106909213700454528 099.53163508451 -01.46839862892 11.0128 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 51886_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 51886_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (228.6") between the two second-epoch detections
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Considering the candidate 54100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 54100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (303.5") between the two second-epoch detections
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Considering the candidate 54900_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 54900_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:37.39 -03:49:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57145_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57145_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:09.79 -02:35:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 2.899 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57309_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57309_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (247.1") between the two second-epoch detections
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Considering the candidate 57312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:44:47.79 -05:17:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57460_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57460_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:06.03 -01:21:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.939 3106351868685803136 102.77430949376 -01.36248533429 11.9159 11.5174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57533_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57533_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:44.25 -02:34:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.385 3106104714788050432 101.93458736101 -02.57691600924 12.0161 11.7182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57601_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57601_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:36:18.05 -05:48:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 4.344 3103232515541099520 099.07422740853 -05.81032084959 11.4256 10.3522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57726_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57726_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (43.4") between the two second-epoch detections
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Considering the candidate 57776_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57776_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:36.27 -02:12:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.646 3106608119313089792 100.65078624539 -02.20722417901 11.9774 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57879_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57879_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:02.01 -01:58:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.155 3106243184533303808 102.50792666588 -01.97042486853 12.1654 12.0227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57896_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57896_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:23.97 -02:34:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57943_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57943_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:54.57 -02:39:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.599 3106089046747361664 102.22766189689 -02.66193005359 12.0134 11.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57961_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 57961_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:34.28 -03:48:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.813 3102724167510104832 103.14279316924 -03.80500207540 12.0938 11.8556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 58156_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 58156_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:50.06 -05:33:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.583 3101894379828642944 102.95915856284 -05.56087713298 11.9962 11.6123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 58240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 58240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (58.1") between the two second-epoch detections
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Considering the candidate 58412_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 58412_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:09.49 -03:38:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.406 3105417661758290432 102.53901700476 -03.64244311062 11.8268 10.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58499_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 58499_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (159.1") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Image size: 925.0'x622.6' 15.4(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.85"/pix along the Y axis
Image center: 06:51:30.811 -01:59:12.56 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 06:51:30.811 -01:59:12.56
Angular distance between the image centers 0.0541 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:32.084 -01:59:53.91 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 06:51:32.084 -01:59:53.91
Angular distance between the image centers 0.0462 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 06:51:30.811 -01:59:12.56
Second-epoch second image center 06:51:32.084 -01:59:53.91
Angular distance between the image centers 0.01265 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.HFLvLxXjJB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.g3rybZDd6I
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits &> /tmp/tmp.ZgtyLCvlDP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits &> /tmp/tmp.Mp319Ets2m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 465 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.1 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
14.1 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HFLvLxXjJB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.g3rybZDd6I (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZgtyLCvlDP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=93, blended=33946, passed=209325
Got 209325 stars (including 175142 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 209325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 925.0'
Seting catalog search parameters based on the expected field of view 925.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012847 (46.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010278 (37.0 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 676 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 613 matched stars entering correct_measured_positions(), 106649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.05"
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 713 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 677 matched stars entering correct_measured_positions(), 106671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.05"
Accuracy estimation diagnostic: 674 matched stars entering correct_measured_positions(), 118632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.76"
Excluding outliers - 674 stars left (next iteration limit 674)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.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.Mp319Ets2m (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=33992, passed=209053
Got 209053 stars (including 174830 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 209053 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 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: 932 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 205661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 205662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 205665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 930 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-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-36-32_20.00sec_-4.90C_LIGHT_0035.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_220449_TTUQ2b1x1_20488_IO9apEzg/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out283716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out328810.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out273991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out287457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330408.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 172s
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: 82s
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Considering the candidate 283692_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283692_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (260.3") between the two second-epoch detections
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Considering the candidate 283702_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283702_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (164.6") between the two second-epoch detections
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Considering the candidate 283705_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283705_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283710_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283710_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283713_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283713_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (163.5") between the two second-epoch detections
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Considering the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283716_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:09.72 -02:45:30.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283735_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283735_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (96.8") between the two second-epoch detections
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Considering the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283741_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (159.1") between the two second-epoch detections
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Considering the candidate 283743_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283743_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (154.8") between the two second-epoch detections
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Considering the candidate 283747_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283747_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283753_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283753_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283760_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283760_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (232.9") between the two second-epoch detections
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Considering the candidate 283763_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283763_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (249.9") between the two second-epoch detections
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Considering the candidate 283765_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283765_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283766_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283766_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (151.0") between the two second-epoch detections
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Considering the candidate 283767_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283767_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283769_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:51.57 -00:02:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.348 3119634445885288832 099.71366987604 -00.03469686871 14.6888 14.1258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283771_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283771_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (154.6") between the two second-epoch detections
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Considering the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283774_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283774_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:12.02 +00:14:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.279 3125505704838714496 101.29941187509 +00.23685264125 14.4374 13.9985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283782_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283782_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283786_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283786_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283787_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283787_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (186.8") between the two second-epoch detections
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Considering the candidate 283790_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283790_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (257.8") between the two second-epoch detections
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283803_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 283805_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283805_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (162.6") between the two second-epoch detections
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Considering the candidate 283810_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283810_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (256.1") between the two second-epoch detections
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Considering the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283816_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (216.7") between the two second-epoch detections
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Considering the candidate 283818_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283818_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283832_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283832_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283833_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (144.7") between the two second-epoch detections
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Considering the candidate 283838_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283838_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:42.27 -04:19:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.677 3102317691803736448 102.92545757643 -04.32463577603 14.5514 14.0466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283843_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283843_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (256.1") between the two second-epoch detections
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Considering the candidate 283850_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283850_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:59.43 +00:54:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 5.544 3119847648062126464 099.99654025840 +00.91468433371 13.2693 11.8723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283855_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283855_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283862_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283862_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283866_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283866_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (86.8") between the two second-epoch detections
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Considering the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283869_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (199.8") between the two second-epoch detections
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Considering the candidate 283870_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283870_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283872_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (292.5") between the two second-epoch detections
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Considering the candidate 283888_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283888_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (269.6") between the two second-epoch detections
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Considering the candidate 283889_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283889_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:43:02.37 -01:07:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.072 3107262298675097344 100.75895055223 -01.13081862188 14.4695 13.5928 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 283890_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283890_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (133.8") between the two second-epoch detections
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Considering the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283903_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (37.6") between the two second-epoch detections
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Considering the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283906_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:37:56.14 +00:48:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.333 3119831739505299200 099.48321128109 +00.80041368826 14.1506 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283916_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283916_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (211.8") between the two second-epoch detections
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Considering the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283924_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283924_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:42.17 -02:57:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 283926_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283926_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (119.1") between the two second-epoch detections
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Considering the candidate 283938_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283938_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283942_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283942_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (101.3") between the two second-epoch detections
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Considering the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283947_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283947_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (144.7") between the two second-epoch detections
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Considering the candidate 283959_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283959_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (99.6") between the two second-epoch detections
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Considering the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283963_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (67.0") between the two second-epoch detections
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Considering the candidate 283972_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 283972_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283982_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (89.2") between the two second-epoch detections
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Considering the candidate 283994_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 283994_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (105.7") between the two second-epoch detections
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Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284000_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:53:03.04 +01:17:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.668 3114067687234902528 103.26150189626 +01.29007914832 14.2536 13.7674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284002_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284002_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (243.1") between the two second-epoch detections
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Considering the candidate 284004_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284004_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284005_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284005_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:17.58 -04:22:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.801 3102314118390911104 103.07205510738 -04.37743286407 14.1845 13.6979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284013_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284013_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 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 284017_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284017_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (320.5") between the two second-epoch detections
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Considering the candidate 284019_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284019_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:36:00.23 -01:43:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.848 3118793942263638400 099.00070840221 -01.72803940748 13.7274 13.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284022_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284022_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284027_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284027_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (242.2") between the two second-epoch detections
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Considering the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284029_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:46.12 -03:39:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.347 3104854540005927040 099.69109841046 -03.66406703747 13.7156 12.8041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284031_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284031_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (171.9") between the two second-epoch detections
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Considering the candidate 284037_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284037_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
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Considering the candidate 284038_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284038_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (57.0") between the two second-epoch detections
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Considering the candidate 284041_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284041_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (243.1") between the two second-epoch detections
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Considering the candidate 284042_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284042_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (224.2") between the two second-epoch detections
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Considering the candidate 284043_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284043_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:53.46 +01:01:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.474 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284045_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284045_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (138.3") between the two second-epoch detections
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Considering the candidate 284047_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284047_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284054_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284054_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 284065_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284065_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (90.8") between the two second-epoch detections
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Considering the candidate 284066_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284066_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:14.71 -05:48:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284069_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:49.08 +01:08:52.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 284070_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284070_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284076_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284076_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284079_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284079_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (189.8") between the two second-epoch detections
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Considering the candidate 284081_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284081_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:56:27.88 -01:27:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.538 3112108086934928000 104.11563795196 -01.45771740901 13.9393 13.2791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284082_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284082_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (213.4") between the two second-epoch detections
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Considering the candidate 284087_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284087_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284090_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284090_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:02.40 +01:08:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.399 3125863454135067008 100.25961682602 +01.14441492507 14.1205 13.5264 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 284094_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284094_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (40.0") between the two second-epoch detections
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Considering the candidate 284096_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284096_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284102_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284102_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (108.0") between the two second-epoch detections
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Considering the candidate 284103_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284103_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (210.1") between the two second-epoch detections
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Considering the candidate 284107_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284107_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (46.6") between the two second-epoch detections
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Considering the candidate 284108_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284108_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (335.1") between the two second-epoch detections
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Considering the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284112_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (208.6") between the two second-epoch detections
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Considering the candidate 284117_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284117_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284119_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284119_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (268.8") between the two second-epoch detections
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Considering the candidate 284120_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284120_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (242.3") between the two second-epoch detections
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Considering the candidate 284121_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284121_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (289.4") between the two second-epoch detections
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Considering the candidate 284123_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284123_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:00.98 -04:47:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.575 3103871267373554944 099.75380851897 -04.78538286533 13.9606 13.4138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284126_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284126_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284127_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (121.3") between the two second-epoch detections
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Considering the candidate 284129_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284129_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (124.3") between the two second-epoch detections
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Considering the candidate 284130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284131_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284131_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:43:11.76 -02:02:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.911 3106617259003491456 100.79850991076 -02.03450460142 13.7064 13.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284137_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284137_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 284140_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284140_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (54.5") between the two second-epoch detections
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Considering the candidate 284141_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284141_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (269.8") between the two second-epoch detections
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Considering the candidate 284142_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284142_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:02.92 -03:47:43.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 284144_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284144_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 284146_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284146_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (88.3") between the two second-epoch detections
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Considering the candidate 284147_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284147_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (375.6") between the two second-epoch detections
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Considering the candidate 284148_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284148_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (132.7") between the two second-epoch detections
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Considering the candidate 284158_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284158_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (36.8") between the two second-epoch detections
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Considering the candidate 284159_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284159_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (176.0") between the two second-epoch detections
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Considering the candidate 284160_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284160_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (300.5") between the two second-epoch detections
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Considering the candidate 284166_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284166_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (175.8") between the two second-epoch detections
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Considering the candidate 284170_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284170_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (261.4") between the two second-epoch detections
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Considering the candidate 284172_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284172_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:37.61 -02:21:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.571 3106690204730551936 099.65602265592 -02.35585984284 13.2484 12.1574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284173_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284173_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (186.9") between the two second-epoch detections
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Considering the candidate 284175_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284175_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (195.3") between the two second-epoch detections
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Considering the candidate 284179_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284179_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:44.37 +00:27:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.472 3119584108871539072 100.43410634763 +00.45760760434 13.7271 13.1248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284197_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284197_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:23.96 -05:15:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.673 3101964366313335296 102.59896228734 -05.26153723479 13.5496 13.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (185.1") between the two second-epoch detections
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Considering the candidate 284204_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284204_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284209_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284209_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:22.60 +00:57:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.367 3113981792187414656 103.09343035440 +00.95023047930 13.5548 12.9216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284210_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284210_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (103.8") between the two second-epoch detections
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Considering the candidate 284221_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284221_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (125.3") between the two second-epoch detections
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Considering the candidate 284222_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284222_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:44:18.49 -05:27:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.711 3100667290492598144 101.07632058798 -05.45614390659 13.5828 13.1018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284224_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284224_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (223.0") between the two second-epoch detections
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Considering the candidate 284226_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284226_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (122.3") between the two second-epoch detections
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Considering the candidate 284228_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284228_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (56.9") between the two second-epoch detections
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Considering the candidate 284232_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284232_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284236_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284236_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:50.01 +00:22:45.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 284238_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284238_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (254.1") between the two second-epoch detections
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Considering the candidate 284244_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284244_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:57:53.21 -00:24:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.540 3112475323818314752 104.47188036842 -00.41113470113 13.3040 12.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284245_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284245_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284246_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284246_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (328.7") between the two second-epoch detections
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Considering the candidate 284248_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284248_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (281.7") between the two second-epoch detections
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Considering the candidate 284249_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284249_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:12.72 +00:51:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284251_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284251_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (219.1") between the two second-epoch detections
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Considering the candidate 284253_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284253_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (47.3") between the two second-epoch detections
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Considering the candidate 284254_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284254_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (288.1") between the two second-epoch detections
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Considering the candidate 284255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (137.3") between the two second-epoch detections
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Considering the candidate 284256_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284256_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284264_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284264_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 284268_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284268_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284275_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284275_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (322.2") between the two second-epoch detections
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Considering the candidate 284276_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284276_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (238.5") between the two second-epoch detections
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Considering the candidate 284277_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284277_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:09.88 -03:38:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.777 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284282_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284282_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284286_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284286_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (48.1") between the two second-epoch detections
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Considering the candidate 284288_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284288_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (232.4") between the two second-epoch detections
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Considering the candidate 284291_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284291_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (27.1") between the two second-epoch detections
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Considering the candidate 284295_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284295_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (193.6") between the two second-epoch detections
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Considering the candidate 284300_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284300_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (225.7") between the two second-epoch detections
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Considering the candidate 284301_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284301_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:53:50.87 +01:53:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284302_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284302_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:55:19.35 -02:31:02.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)
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Considering the candidate 284308_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284308_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284309_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284309_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284310_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284310_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (284.6") between the two second-epoch detections
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Considering the candidate 284312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (229.2") between the two second-epoch detections
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Considering the candidate 284313_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284313_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 284314_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 284314_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 284315_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284315_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (250.7") between the two second-epoch detections
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Considering the candidate 284317_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284317_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:53:11.90 -01:33:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 2.971 3112276892032630400 103.29879130350 -01.56062176551 12.3437 11.9261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284318_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284318_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (253.2") between the two second-epoch detections
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Considering the candidate 284320_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284320_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (39.4") between the two second-epoch detections
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Considering the candidate 284321_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284321_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (345.6") between the two second-epoch detections
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Considering the candidate 284326_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 284326_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (326.0") between the two second-epoch detections
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Considering the candidate 287457_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 287457_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 289065_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 289065_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:37.27 +00:27:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289551_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 289551_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:39.81 +00:25:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289910_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 289910_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 290848_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 290848_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:37.84 +00:43:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291103_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 291103_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:30.63 -01:04:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291209_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 291209_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (171.8") between the two second-epoch detections
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Considering the candidate 292129_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 292129_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:41.75 -00:33:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293567_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 293567_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (65.3") between the two second-epoch detections
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Considering the candidate 293677_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 293677_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (139.9") between the two second-epoch detections
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Considering the candidate 294111_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 294111_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (213.2") between the two second-epoch detections
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Considering the candidate 299220_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 299220_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (289.3") between the two second-epoch detections
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Considering the candidate 299240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 299240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:35:16.50 -04:45:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 299553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:00.29 -00:03:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 301376_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 301376_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (73.9") between the two second-epoch detections
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Considering the candidate 301590_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 301590_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (244.2") between the two second-epoch detections
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Considering the candidate 301902_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 301902_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (216.1") between the two second-epoch detections
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Considering the candidate 301994_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 301994_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:54.40 +00:00:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.970 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302070_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 302070_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:17.70 -04:25:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.732 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302218_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 302218_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:04.93 -01:02:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 4.281 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302638_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 302638_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:34:15.18 -05:19:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 4.624 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302652_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 302652_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (251.1") between the two second-epoch detections
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Considering the candidate 302735_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 302735_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (308.6") between the two second-epoch detections
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Considering the candidate 303414_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 303414_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
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Considering the candidate 303488_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 303488_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (112.4") between the two second-epoch detections
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Considering the candidate 303991_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 303991_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (309.2") between the two second-epoch detections
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Considering the candidate 304133_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 304133_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (130.3") between the two second-epoch detections
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Considering the candidate 304875_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 304875_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 305016_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 305016_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:03.91 -03:46:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305177_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 305177_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:06.19 -00:02:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.218 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305990_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 305990_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 306112_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 306112_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:54:23.57 -01:37:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.228 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306624_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 306624_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 306709_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 306709_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 306728_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 306728_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 306982_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 306982_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:14.19 -00:06:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.126 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307313_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 307313_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 307533_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 307533_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 307555_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 307555_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:36.11 +01:59:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308193_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 308193_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 308279_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308279_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:18.65 -00:51:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.052 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308498_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308498_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 308515_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308515_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (233.4") between the two second-epoch detections
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Considering the candidate 308553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (72.8") between the two second-epoch detections
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Considering the candidate 308842_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308842_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:44:26.43 -06:06:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.667 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 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 308981_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 308981_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:56:43.47 +02:11:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309145_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 309145_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (266.1") between the two second-epoch detections
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Considering the candidate 309350_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 309350_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 309355_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 309355_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (186.0") between the two second-epoch detections
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Considering the candidate 310844_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 310844_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:30.68 +00:57:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.626 3125654791743165184 102.12743384694 +00.96221421685 13.6988 13.2550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310967_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 310967_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (68.3") between the two second-epoch detections
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Considering the candidate 311279_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 311279_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:26.05 -01:49:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.576 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311500_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 311500_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:21.20 -03:11:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.266 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311612_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 311612_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (254.1") between the two second-epoch detections
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Considering the candidate 311703_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 311703_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:25.20 +00:07:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.804 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311716_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 311716_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:33.49 +01:51:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 312342_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 312342_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (238.3") between the two second-epoch detections
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Considering the candidate 312361_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 312361_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 312406_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 312406_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 312408_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 312408_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:20.50 -05:15:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.071 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312872_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 312872_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (48.4") between the two second-epoch detections
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Considering the candidate 312934_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 312934_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (54.7") between the two second-epoch detections
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Considering the candidate 312984_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 312984_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:26.34 -02:20:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.476 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313119_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313119_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (68.2") between the two second-epoch detections
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Considering the candidate 313296_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 313296_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 313337_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313337_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:46.57 -02:44:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.460 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313627_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313627_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (106.3") between the two second-epoch detections
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Considering the candidate 313657_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313657_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (99.9") between the two second-epoch detections
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Considering the candidate 313792_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313792_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:29.81 -04:08:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.922 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313864_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 313864_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 313867_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 313867_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 313896_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 313896_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 313955_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313955_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:05.65 -05:41:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 5.728 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313978_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 313978_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:53.22 +01:49:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.823 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314299_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 314299_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 314469_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 314469_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 314510_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314510_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (130.6") between the two second-epoch detections
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Considering the candidate 314534_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 314534_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 314553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314553_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (108.6") between the two second-epoch detections
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Considering the candidate 314636_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314636_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:12.72 -05:08:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.724 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 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 314664_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 314664_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 314678_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314678_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:48.82 -04:02:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.158 3102343049290484992 102.95330842454 -04.04267620034 13.9995 13.2065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314709_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314709_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:35:10.57 -00:43:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.582 3119206774519517696 098.79348040669 -00.72377880410 14.0197 13.4537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314736_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314736_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (173.4") between the two second-epoch detections
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Considering the candidate 314766_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314766_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:04.25 +01:58:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314792_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 314792_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 314890_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314890_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:55:12.74 +01:46:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (39.6") between the two second-epoch detections
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Considering the candidate 314935_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314935_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:55:58.83 -01:35:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.870 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314969_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 314969_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:33.83 -00:26:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.672 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315046_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 315046_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (242.6") between the two second-epoch detections
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Considering the candidate 315565_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 315565_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:54:23.22 -02:46:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.702 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315658_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 315658_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 315671_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 315671_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:54.76 +02:12:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315703_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 315703_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:01.88 +00:15:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.978 3113554838079394432 102.50697226187 +00.24994566152 13.7718 12.8036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315772_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 315772_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (222.5") between the two second-epoch detections
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Considering the candidate 316086_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316086_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (211.2") between the two second-epoch detections
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Considering the candidate 316107_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 316107_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 316265_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316265_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:36:19.12 +00:01:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.413 3119670321748998144 099.07841400793 +00.02333476458 13.6081 12.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316393_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316393_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:28.93 -06:01:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.177 3103166480420332032 099.61974936398 -06.02795289401 13.7856 12.9545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316426_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 316426_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 316429_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316429_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (253.9") between the two second-epoch detections
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Considering the candidate 316603_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 316603_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 316622_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316622_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (115.7") between the two second-epoch detections
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Considering the candidate 316654_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 316654_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 316777_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316777_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (68.2") between the two second-epoch detections
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Considering the candidate 316830_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316830_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (108.8") between the two second-epoch detections
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Considering the candidate 316881_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 316881_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:41.26 +00:31:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.935 3113534565832235008 101.92116485332 +00.52468696916 14.0518 13.5241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317006_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 317006_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 317038_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 317038_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (214.8") between the two second-epoch detections
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Considering the candidate 317254_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 317254_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 317640_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 317640_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (270.1") between the two second-epoch detections
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Considering the candidate 317652_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 317652_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:08.84 -03:48:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.462 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317743_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 317743_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (111.9") between the two second-epoch detections
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Considering the candidate 317782_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 317782_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:27.84 +01:39:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.414 3126135209605384448 102.36549196435 +01.66385619264 14.1154 13.6175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 318130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 318150_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 318150_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 318366_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 318366_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (143.5") between the two second-epoch detections
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Considering the candidate 318581_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 318581_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (281.3") between the two second-epoch detections
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Considering the candidate 318585_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 318585_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (137.9") between the two second-epoch detections
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Considering the candidate 318814_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 318814_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 318918_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 318918_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:52.51 +01:12:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.097 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319301_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319301_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:44.20 -05:54:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.705 3100366264824580480 102.18279250022 -05.90788495291 13.4790 12.3244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319307_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319307_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (197.3") between the two second-epoch detections
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Considering the candidate 319360_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 319360_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 319524_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319524_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:36:24.62 -01:37:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.663 3118888878221465216 099.10208805229 -01.62577794876 14.0413 13.4585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319574_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319574_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (282.3") between the two second-epoch detections
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Considering the candidate 319705_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319705_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:47.14 -00:07:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.704 3113468973092058240 101.69553406151 -00.13282456161 14.0572 13.1422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319753_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 319753_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 319811_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319811_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (132.7") between the two second-epoch detections
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Considering the candidate 319961_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 319961_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 320473_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 320473_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 320714_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 320714_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 320798_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 320798_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 320834_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 320834_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:24.77 -00:56:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.224 3107130769594752128 102.35183201837 -00.93873825599 14.2056 13.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321235_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 321235_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 321259_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321259_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:44:01.13 -05:45:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.736 3100606576835105152 101.00414373612 -05.76059468454 14.4179 13.5852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321327_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321327_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (60.6") between the two second-epoch detections
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Considering the candidate 321450_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321450_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (148.3") between the two second-epoch detections
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Considering the candidate 321468_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 321468_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 321487_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 321487_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 321498_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321498_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:15.56 +01:14:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.724 3125885414305835648 100.56374559839 +01.24197894342 13.9411 13.1211 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 321647_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321647_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:38.89 +00:36:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.419 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321683_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321683_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:57.57 -02:12:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.311 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321732_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 321732_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 321807_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321807_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (76.3") between the two second-epoch detections
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Considering the candidate 321821_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 321821_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 321851_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 321851_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:27.25 -05:52:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.791 3101108916207784960 103.11340523708 -05.87976646569 14.0840 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322017_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322017_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:52.04 -04:03:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 4.112 3102342980571017472 102.96630269222 -04.06398447247 14.2492 13.7474 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 322031_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 322031_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 322046_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322046_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (57.6") between the two second-epoch detections
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Considering the candidate 322120_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322120_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:57.17 -04:34:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.268 3103787734552535808 100.23751504165 -04.58187315124 14.1352 13.3718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 322199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 322570_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322570_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 322661_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322661_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (66.7") between the two second-epoch detections
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Considering the candidate 322696_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 322696_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 322769_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 322769_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (244.6") between the two second-epoch detections
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Considering the candidate 322895_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 322895_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 322973_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 322973_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 323100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323100_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (315.4") between the two second-epoch detections
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Considering the candidate 323369_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323369_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (61.3") between the two second-epoch detections
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Considering the candidate 323389_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323389_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:53.58 -00:49:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.361 3119330641377186688 099.72224575617 -00.82187219144 14.2480 13.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323394_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323394_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:51:34.35 -02:33:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.952 3106011535478207360 102.89197053929 -02.55502747934 14.0434 13.2003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323531_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323531_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:49.27 -05:38:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.425 3100435534056353152 101.70542790137 -05.64395521384 14.2234 13.3872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323603_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 323603_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:46:39.67 -05:23:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.291 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323947_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 323947_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 324172_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 324172_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (130.1") between the two second-epoch detections
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Considering the candidate 324539_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 324539_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 324546_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 324546_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 324946_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 324946_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (102.7") between the two second-epoch detections
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Considering the candidate 325006_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 325006_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 325097_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 325097_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 325190_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 325190_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:38.20 -00:17:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.086 3119433956814456704 099.65819127034 -00.29763616830 14.2367 13.6075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 325255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:11.54 -00:25:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.098 3113216669534339456 102.29729293236 -00.42701368548 14.4407 13.9401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325334_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 325334_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 325630_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 325630_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:35:16.81 -01:19:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.750 3118957632057909376 098.81878136857 -01.31878064928 14.3099 13.6904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325729_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 325729_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (191.7") between the two second-epoch detections
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Considering the candidate 325821_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 325821_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:53:47.96 +00:29:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.519 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326214_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326214_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:16.61 +01:20:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.104 3125879435710966400 100.31840771403 +01.33635738412 14.4688 13.9082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326444_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326444_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (53.4") between the two second-epoch detections
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Considering the candidate 326503_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326503_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (135.6") between the two second-epoch detections
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Considering the candidate 326507_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 326507_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 326524_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326524_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:37:19.38 +00:16:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.226 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326730_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326730_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (202.3") between the two second-epoch detections
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Considering the candidate 326794_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326794_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (246.2") between the two second-epoch detections
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Considering the candidate 326914_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326914_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (136.0") between the two second-epoch detections
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Considering the candidate 326956_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 326956_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (46.2") between the two second-epoch detections
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Considering the candidate 327012_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327012_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:22.41 +01:18:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.530 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327045_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327045_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (245.1") between the two second-epoch detections
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Considering the candidate 327053_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327053_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:34:54.53 +01:23:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.501 3120676855925773696 098.72578573357 +01.39802428046 13.2177 11.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327277_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327277_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 327392_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327392_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:44:43.34 -02:05:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.379 3106941413077711360 101.17994342396 -02.10121165387 14.0609 13.1706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327487_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327487_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:45:44.12 -05:21:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.188 3100647018246730496 101.43271567135 -05.36629970512 14.4549 13.5997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327509_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327509_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (99.1") between the two second-epoch detections
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Considering the candidate 327563_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327563_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:48:38.57 +01:00:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.666 3125656093114494464 102.15981419286 +01.00036730696 14.3881 13.7184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327591_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327591_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:24.50 -01:03:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.887 3107126508988092544 102.35130968936 -01.05111434072 14.5931 13.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327620_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327620_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (262.2") between the two second-epoch detections
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Considering the candidate 327677_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327677_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (140.4") between the two second-epoch detections
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Considering the candidate 327760_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327760_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (210.7") between the two second-epoch detections
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Considering the candidate 327806_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327806_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:40:47.50 -04:08:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 5.411 3104027088786480640 100.19665296976 -04.14401316026 14.4759 13.8163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327808_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327808_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (261.4") between the two second-epoch detections
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Considering the candidate 327873_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327873_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (303.6") between the two second-epoch detections
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Considering the candidate 327908_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327908_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:50.50 +00:03:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.326 3113500721490740224 101.95952954964 +00.05332490721 14.5611 13.5877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327935_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327935_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:56:22.03 -01:52:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.961 3112020950638770688 104.09149206320 -01.88276179988 14.5685 14.0348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327946_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327946_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (235.3") between the two second-epoch detections
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Considering the candidate 327978_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 327978_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 327979_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 327979_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 327993_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 327993_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 327998_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 327998_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328051_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328051_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:49:52.18 +00:49:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.927 3113659944517871104 102.46656884662 +00.83187008901 14.3851 13.8439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 328202_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328202_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (247.3") between the two second-epoch detections
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Considering the candidate 328217_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328217_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:33:29.10 +01:58:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.611 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 328310_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328310_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (242.6") between the two second-epoch detections
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Considering the candidate 328347_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328347_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:38:37.59 +01:13:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 5.025 3120622979856518400 099.65577942531 +01.21841698575 14.7206 14.2540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 328495_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 328495_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328549_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 328549_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328615_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328615_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (141.4") between the two second-epoch detections
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Considering the candidate 328718_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 328718_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328738_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 328738_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328810_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328810_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:05.71 +00:51:27.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 328834_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 328834_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 328847_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328847_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 328894_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328894_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:04.25 -05:07:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.971 3103692356216888704 100.51710199007 -05.12513063757 14.3238 13.4888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 328951_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 328951_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (92.5") between the two second-epoch detections
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Considering the candidate 329039_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329039_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (151.4") between the two second-epoch detections
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Considering the candidate 329110_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329110_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (59.6") between the two second-epoch detections
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Considering the candidate 329199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329199_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (58.3") between the two second-epoch detections
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Considering the candidate 329245_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329245_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (161.4") between the two second-epoch detections
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Considering the candidate 329263_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329263_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (277.6") between the two second-epoch detections
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Considering the candidate 329319_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329319_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (161.0") between the two second-epoch detections
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Considering the candidate 329329_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329329_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329354_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329354_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (330.6") between the two second-epoch detections
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Considering the candidate 329372_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329372_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329396_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329396_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329448_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329448_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (238.0") between the two second-epoch detections
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Considering the candidate 329458_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329458_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (327.2") between the two second-epoch detections
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Considering the candidate 329462_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329462_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:54:52.31 -02:37:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.255 3105971334584697216 103.71669581737 -02.62504076135 13.9313 12.7828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 329532_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329532_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (268.0") between the two second-epoch detections
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Considering the candidate 329549_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329549_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329606_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329606_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 329613_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329613_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (239.0") between the two second-epoch detections
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Considering the candidate 329631_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329631_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (130.9") between the two second-epoch detections
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Considering the candidate 329646_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329646_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329669_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329669_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329707_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329707_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:52:04.07 -01:15:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.589 3112347436873213568 103.01632428710 -01.25860600229 14.6296 14.1000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 329734_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329734_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:39:46.26 -02:13:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.513 3106783152122101120 099.94209701518 -02.23397557183 14.5512 13.9164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 329820_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329820_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (129.0") between the two second-epoch detections
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Considering the candidate 329824_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329824_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:47:01.53 -05:25:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.558 3100633514869428224 101.75545382235 -05.42849190189 14.2726 13.3215 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 329826_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329826_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329827_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329827_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (324.8") between the two second-epoch detections
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Considering the candidate 329871_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329871_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (257.3") between the two second-epoch detections
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Considering the candidate 329880_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329880_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (68.3") between the two second-epoch detections
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Considering the candidate 329928_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329928_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:34:48.99 -00:10:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.255 3119662350289897728 098.70332506390 -00.18198105991 14.5966 13.9457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 329936_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 329936_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (119.3") between the two second-epoch detections
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Considering the candidate 329971_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329971_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 329997_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 329997_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330026_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330026_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (166.0") between the two second-epoch detections
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Considering the candidate 330052_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330052_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (120.7") between the two second-epoch detections
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Considering the candidate 330108_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330108_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (44.6") between the two second-epoch detections
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Considering the candidate 330114_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330114_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (248.7") between the two second-epoch detections
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Considering the candidate 330130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330130_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (308.1") between the two second-epoch detections
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Considering the candidate 330160_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330160_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330181_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330181_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330212_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330212_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 330225_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330225_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (130.9") between the two second-epoch detections
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Considering the candidate 330238_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330238_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (220.6") between the two second-epoch detections
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Considering the candidate 330240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330240_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (140.5") between the two second-epoch detections
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Considering the candidate 330246_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330246_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (48.4") between the two second-epoch detections
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Considering the candidate 330255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330255_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330259_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330259_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330261_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330261_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (248.4") between the two second-epoch detections
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Considering the candidate 330267_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330267_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (231.6") between the two second-epoch detections
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Considering the candidate 330283_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330283_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (43.0") between the two second-epoch detections
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Considering the candidate 330288_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330288_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (293.1") between the two second-epoch detections
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Considering the candidate 330312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330312_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:42:37.12 +00:32:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.371 3125587584094432896 100.65443782324 +00.53870311297 14.7626 14.2244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 330336_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330336_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (68.1") between the two second-epoch detections
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Considering the candidate 330357_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330357_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330387_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330387_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:43:00.52 -04:32:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.124 3103799111923579648 100.75114026978 -04.54290592547 14.5489 13.9881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 330408_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 330408_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
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Considering the candidate 330441_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330441_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (178.0") between the two second-epoch detections
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Considering the candidate 330485_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330485_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 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 330501_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330501_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (87.7") between the two second-epoch detections
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Considering the candidate 330527_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330527_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 330632_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 330632_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (340.6") between the two second-epoch detections
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:50:00.85 +01:46:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 273991_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
Preparing report for the candidate 273991_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (292.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
Rejecting candidate due to large distance (248.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:41:59.38 -01:11:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-15_21-37-22_20.00sec_-4.90C_LIGHT_0036 did not pass the final checks
**** FOUND 06:37:53.29 -05:55:14.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 261s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:52:06.36 -01:18:21.3
06:51:22.49 +00:33:44.7
06:54:46.92 -00:18:59.3
06:56:09.54 +00:41:04.9
06:44:26.10 +01:22:07.5
06:46:42.50 -05:03:51.9
06:48:21.59 +01:48:28.8
06:50:54.65 -00:02:39.5
06:53:24.31 -05:41:34.5
06:55:10.87 -00:02:52.8
06:51:10.27 -01:42:51.2
06:46:19.49 -01:57:13.3
06:44:50.62 -04:52:04.6
06:40:15.52 +00:55:17.2
06:43:14.36 +01:58:18.4
06:56:45.61 -01:04:28.3
06:56:16.28 -01:49:27.8
06:57:12.84 +00:55:21.6
06:53:43.72 -01:58:41.7
06:55:40.69 -00:18:32.3
06:56:38.45 -01:07:56.9
06:47:20.72 -05:40:15.0
06:46:31.08 +01:08:33.8
06:53:52.41 -02:12:23.2
06:53:04.64 -05:33:23.2
06:55:37.02 -01:03:22.4
06:43:22.36 +01:54:49.3
06:56:17.34 +00:50:17.0
06:46:25.60 -00:28:37.8
06:55:10.99 -02:39:48.4
06:44:25.53 +01:06:41.9
06:50:24.04 -01:20:43.3
06:48:46.70 +01:42:52.1
06:53:36.93 -02:31:47.8
06:49:52.51 -02:39:52.3
06:46:14.03 +00:50:43.4
06:35:07.51 -03:03:03.8
06:51:26.12 -01:48:02.1
06:53:04.25 -00:08:10.5
06:44:34.17 -01:35:28.4
06:43:27.89 -03:56:30.7
06:53:50.88 -00:03:51.8
06:51:33.03 +00:27:11.8
06:45:12.41 -00:01:51.8
06:50:14.58 -00:47:13.2
06:54:48.61 +00:23:18.5
06:42:39.21 -02:16:09.0
06:41:58.95 -02:54:56.4
06:52:55.21 -02:23:01.3
06:54:43.94 -02:41:21.1
06:55:27.37 -01:16:23.1
06:42:33.31 -03:28:05.3
06:56:11.81 -01:22:23.1
06:49:07.53 -01:40:18.1
06:41:27.19 -01:19:02.1
06:54:42.07 -02:41:59.4
06:46:50.75 +01:18:08.1
06:51:34.45 -01:39:22.7
06:50:18.23 +00:24:41.2
06:52:36.44 -02:12:52.8
06:50:34.46 -02:44:34.8
06:49:56.12 -02:17:03.6
06:42:31.13 -06:04:20.9
06:36:32.51 -03:35:54.2
06:43:55.64 -05:04:02.0
06:53:41.64 -00:33:48.7
06:47:09.69 -05:17:17.4
06:57:35.50 +01:13:54.9
06:50:41.61 -00:31:44.4
06:45:54.19 -00:09:37.9
06:47:12.07 +00:21:19.1
06:41:21.26 -01:43:18.9
06:38:58.68 -00:30:12.9
06:43:37.06 -04:25:01.6
06:50:08.50 +00:46:16.9
06:45:17.72 +00:43:40.6
06:48:23.40 -05:30:23.9
06:48:34.77 -03:13:30.5
06:55:16.14 +00:20:57.7
06:54:03.57 +02:06:10.4
06:52:34.75 +00:32:33.5
06:53:47.58 -02:38:44.1
06:49:21.41 +01:13:45.9
06:46:32.70 -01:51:11.6
06:44:38.40 -02:01:19.2
06:41:21.42 -00:35:22.3
06:48:12.25 -00:18:59.0
06:56:37.98 +00:11:23.8
06:49:55.03 -04:03:39.1
06:53:59.25 -01:54:57.4
06:55:12.13 +00:56:24.3
06:43:51.37 -04:55:44.4
06:55:50.86 -02:12:28.2
06:46:12.12 +00:43:13.7
06:53:08.29 -00:50:30.0
06:45:22.66 +01:37:11.2
06:51:39.84 -01:26:46.0
06:45:26.28 -00:11:50.6
06:47:53.26 +01:51:22.7
06:55:25.46 +00:38:48.5
06:52:15.24 -03:21:31.5
06:44:26.74 +00:04:54.9
06:51:33.88 -03:50:27.8
06:56:59.96 -00:24:06.2
06:47:10.04 -02:51:22.2
06:42:51.47 -04:30:08.4
06:41:26.98 -01:17:39.9
06:53:03.92 +01:25:47.9
06:52:31.95 -01:11:27.5
06:51:28.97 -01:28:26.1
06:51:21.48 +00:08:53.0
06:51:47.14 -01:07:36.4
06:50:21.65 -05:30:12.5
06:52:00.27 -01:37:37.6
06:55:33.00 +00:42:07.0
06:51:47.89 -00:51:42.9
06:52:19.95 +00:21:27.8
06:51:19.61 -01:48:26.6
06:54:08.45 +01:08:44.0
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:51:22.49 +00:33:44.7
06:54:46.92 -00:18:59.3
06:56:09.54 +00:41:04.9
06:44:26.10 +01:22:07.5
06:46:42.50 -05:03:51.9
06:48:21.59 +01:48:28.8
06:50:54.65 -00:02:39.5
06:53:24.31 -05:41:34.5
06:55:10.87 -00:02:52.8
06:51:10.27 -01:42:51.2
06:46:19.49 -01:57:13.3
06:44:50.62 -04:52:04.6
06:40:15.52 +00:55:17.2
06:43:14.36 +01:58:18.4
06:56:45.61 -01:04:28.3
06:56:16.28 -01:49:27.8
06:57:12.84 +00:55:21.6
06:53:43.72 -01:58:41.7
06:55:40.69 -00:18:32.3
06:56:38.45 -01:07:56.9
06:47:20.72 -05:40:15.0
06:46:31.08 +01:08:33.8
06:53:52.41 -02:12:23.2
06:53:04.64 -05:33:23.2
06:55:37.02 -01:03:22.4
06:43:22.36 +01:54:49.3
06:56:17.34 +00:50:17.0
06:46:25.60 -00:28:37.8
06:55:10.99 -02:39:48.4
06:44:25.53 +01:06:41.9
06:50:24.04 -01:20:43.3
06:48:46.70 +01:42:52.1
06:53:36.93 -02:31:47.8
06:49:52.51 -02:39:52.3
06:46:14.03 +00:50:43.4
06:35:07.51 -03:03:03.8
06:51:26.12 -01:48:02.1
06:53:04.25 -00:08:10.5
06:44:34.17 -01:35:28.4
06:43:27.89 -03:56:30.7
06:53:50.88 -00:03:51.8
06:51:33.03 +00:27:11.8
06:45:12.41 -00:01:51.8
06:50:14.58 -00:47:13.2
06:54:48.61 +00:23:18.5
06:42:39.21 -02:16:09.0
06:41:58.95 -02:54:56.4
06:52:55.21 -02:23:01.3
06:54:43.94 -02:41:21.1
06:55:27.37 -01:16:23.1
06:42:33.31 -03:28:05.3
06:56:11.81 -01:22:23.1
06:49:07.53 -01:40:18.1
06:41:27.19 -01:19:02.1
06:54:42.07 -02:41:59.4
06:46:50.75 +01:18:08.1
06:51:34.45 -01:39:22.7
06:50:18.23 +00:24:41.2
06:52:36.44 -02:12:52.8
06:50:34.46 -02:44:34.8
06:49:56.12 -02:17:03.6
06:42:31.13 -06:04:20.9
06:36:32.51 -03:35:54.2
06:43:55.64 -05:04:02.0
06:53:41.64 -00:33:48.7
06:47:09.69 -05:17:17.4
06:57:35.50 +01:13:54.9
06:50:41.61 -00:31:44.4
06:45:54.19 -00:09:37.9
06:47:12.07 +00:21:19.1
06:41:21.26 -01:43:18.9
06:38:58.68 -00:30:12.9
06:43:37.06 -04:25:01.6
06:50:08.50 +00:46:16.9
06:45:17.72 +00:43:40.6
06:48:23.40 -05:30:23.9
06:48:34.77 -03:13:30.5
06:55:16.14 +00:20:57.7
06:54:03.57 +02:06:10.4
06:52:34.75 +00:32:33.5
06:53:47.58 -02:38:44.1
06:49:21.41 +01:13:45.9
06:46:32.70 -01:51:11.6
06:44:38.40 -02:01:19.2
06:41:21.42 -00:35:22.3
06:48:12.25 -00:18:59.0
06:56:37.98 +00:11:23.8
06:49:55.03 -04:03:39.1
06:53:59.25 -01:54:57.4
06:55:12.13 +00:56:24.3
06:43:51.37 -04:55:44.4
06:55:50.86 -02:12:28.2
06:46:12.12 +00:43:13.7
06:53:08.29 -00:50:30.0
06:45:22.66 +01:37:11.2
06:51:39.84 -01:26:46.0
06:45:26.28 -00:11:50.6
06:47:53.26 +01:51:22.7
06:55:25.46 +00:38:48.5
06:52:15.24 -03:21:31.5
06:44:26.74 +00:04:54.9
06:51:33.88 -03:50:27.8
06:56:59.96 -00:24:06.2
06:47:10.04 -02:51:22.2
06:42:51.47 -04:30:08.4
06:41:26.98 -01:17:39.9
06:53:03.92 +01:25:47.9
06:52:31.95 -01:11:27.5
06:51:28.97 -01:28:26.1
06:51:21.48 +00:08:53.0
06:51:47.14 -01:07:36.4
06:50:21.65 -05:30:12.5
06:52:00.27 -01:37:37.6
06:55:33.00 +00:42:07.0
06:51:47.89 -00:51:42.9
06:52:19.95 +00:21:27.8
06:51:19.61 -01:48:26.6
06:54:08.45 +01:08:44.0
06:52:06.36 -01:18:21.3
###################################################################################
06:51:22.49 +00:33:44.7 -- not an asteroid (will add it to exclusion list)
06:54:46.92 -00:18:59.3 -- not an asteroid (will add it to exclusion list)
06:56:09.54 +00:41:04.9 -- not an asteroid (will add it to exclusion list)
06:44:26.10 +01:22:07.5 -- not an asteroid (will add it to exclusion list)
06:46:42.50 -05:03:51.9 -- not an asteroid (will add it to exclusion list)
06:48:21.59 +01:48:28.8 -- not an asteroid (will add it to exclusion list)
06:50:54.65 -00:02:39.5 -- not an asteroid (will add it to exclusion list)
06:53:24.31 -05:41:34.5 -- not an asteroid (will add it to exclusion list)
06:55:10.87 -00:02:52.8 -- not an asteroid (will add it to exclusion list)
06:51:10.27 -01:42:51.2 -- not an asteroid (will add it to exclusion list)
06:46:19.49 -01:57:13.3 -- not an asteroid (will add it to exclusion list)
06:44:50.62 -04:52:04.6 -- not an asteroid (will add it to exclusion list)
06:40:15.52 +00:55:17.2 -- not an asteroid (will add it to exclusion list)
06:43:14.36 +01:58:18.4 -- not an asteroid (will add it to exclusion list)
06:56:45.61 -01:04:28.3 -- not an asteroid (will add it to exclusion list)
06:56:16.28 -01:49:27.8 -- not an asteroid (will add it to exclusion list)
06:57:12.84 +00:55:21.6 -- not an asteroid (will add it to exclusion list)
06:53:43.72 -01:58:41.7 -- not an asteroid (will add it to exclusion list)
06:55:40.69 -00:18:32.3 -- not an asteroid (will add it to exclusion list)
06:56:38.45 -01:07:56.9 -- not an asteroid (will add it to exclusion list)
06:47:20.72 -05:40:15.0 -- not an asteroid (will add it to exclusion list)
06:46:31.08 +01:08:33.8 -- not an asteroid (will add it to exclusion list)
06:53:52.41 -02:12:23.2 -- not an asteroid (will add it to exclusion list)
06:53:04.64 -05:33:23.2 -- not an asteroid (will add it to exclusion list)
06:55:37.02 -01:03:22.4 -- not an asteroid (will add it to exclusion list)
06:43:22.36 +01:54:49.3 -- not an asteroid (will add it to exclusion list)
06:56:17.34 +00:50:17.0 -- not an asteroid (will add it to exclusion list)
06:46:25.60 -00:28:37.8 -- not an asteroid (will add it to exclusion list)
06:55:10.99 -02:39:48.4 -- not an asteroid (will add it to exclusion list)
06:44:25.53 +01:06:41.9 -- not an asteroid (will add it to exclusion list)
06:50:24.04 -01:20:43.3 -- not an asteroid (will add it to exclusion list)
06:48:46.70 +01:42:52.1 -- not an asteroid (will add it to exclusion list)
06:53:36.93 -02:31:47.8 -- not an asteroid (will add it to exclusion list)
06:49:52.51 -02:39:52.3 -- not an asteroid (will add it to exclusion list)
06:46:14.03 +00:50:43.4 -- not an asteroid (will add it to exclusion list)
06:35:07.51 -03:03:03.8 -- not an asteroid (will add it to exclusion list)
06:51:26.12 -01:48:02.1 -- not an asteroid (will add it to exclusion list)
06:53:04.25 -00:08:10.5 -- not an asteroid (will add it to exclusion list)
06:44:34.17 -01:35:28.4 -- not an asteroid (will add it to exclusion list)
06:43:27.89 -03:56:30.7 -- not an asteroid (will add it to exclusion list)
06:53:50.88 -00:03:51.8 -- not an asteroid (will add it to exclusion list)
06:51:33.03 +00:27:11.8 -- not an asteroid (will add it to exclusion list)
06:45:12.41 -00:01:51.8 -- not an asteroid (will add it to exclusion list)
06:50:14.58 -00:47:13.2 -- not an asteroid (will add it to exclusion list)
06:54:48.61 +00:23:18.5 -- not an asteroid (will add it to exclusion list)
06:42:39.21 -02:16:09.0 -- not an asteroid (will add it to exclusion list)
06:41:58.95 -02:54:56.4 -- not an asteroid (will add it to exclusion list)
06:52:55.21 -02:23:01.3 -- not an asteroid (will add it to exclusion list)
06:54:43.94 -02:41:21.1 -- not an asteroid (will add it to exclusion list)
06:55:27.37 -01:16:23.1 -- not an asteroid (will add it to exclusion list)
06:42:33.31 -03:28:05.3 -- not an asteroid (will add it to exclusion list)
06:56:11.81 -01:22:23.1 -- not an asteroid (will add it to exclusion list)
06:49:07.53 -01:40:18.1 -- not an asteroid (will add it to exclusion list)
06:41:27.19 -01:19:02.1 -- not an asteroid (will add it to exclusion list)
06:54:42.07 -02:41:59.4 -- not an asteroid (will add it to exclusion list)
06:46:50.75 +01:18:08.1 -- not an asteroid (will add it to exclusion list)
06:51:34.45 -01:39:22.7 -- not an asteroid (will add it to exclusion list)
06:50:18.23 +00:24:41.2 -- not an asteroid (will add it to exclusion list)
06:52:36.44 -02:12:52.8 -- not an asteroid (will add it to exclusion list)
06:50:34.46 -02:44:34.8 -- not an asteroid (will add it to exclusion list)
06:49:56.12 -02:17:03.6 -- not an asteroid (will add it to exclusion list)
06:42:31.13 -06:04:20.9 -- not an asteroid (will add it to exclusion list)
06:36:32.51 -03:35:54.2 -- not an asteroid (will add it to exclusion list)
06:43:55.64 -05:04:02.0 -- not an asteroid (will add it to exclusion list)
06:53:41.64 -00:33:48.7 -- not an asteroid (will add it to exclusion list)
06:47:09.69 -05:17:17.4 -- not an asteroid (will add it to exclusion list)
06:57:35.50 +01:13:54.9 -- not an asteroid (will add it to exclusion list)
06:50:41.61 -00:31:44.4 -- not an asteroid (will add it to exclusion list)
06:45:54.19 -00:09:37.9 -- not an asteroid (will add it to exclusion list)
06:47:12.07 +00:21:19.1 -- not an asteroid (will add it to exclusion list)
06:41:21.26 -01:43:18.9 -- not an asteroid (will add it to exclusion list)
06:38:58.68 -00:30:12.9 -- not an asteroid (will add it to exclusion list)
06:43:37.06 -04:25:01.6 -- not an asteroid (will add it to exclusion list)
06:50:08.50 +00:46:16.9 -- not an asteroid (will add it to exclusion list)
06:45:17.72 +00:43:40.6 -- not an asteroid (will add it to exclusion list)
06:48:23.40 -05:30:23.9 -- not an asteroid (will add it to exclusion list)
06:48:34.77 -03:13:30.5 -- not an asteroid (will add it to exclusion list)
06:55:16.14 +00:20:57.7 -- not an asteroid (will add it to exclusion list)
06:54:03.57 +02:06:10.4 -- not an asteroid (will add it to exclusion list)
06:52:34.75 +00:32:33.5 -- not an asteroid (will add it to exclusion list)
06:53:47.58 -02:38:44.1 -- not an asteroid (will add it to exclusion list)
06:49:21.41 +01:13:45.9 -- not an asteroid (will add it to exclusion list)
06:46:32.70 -01:51:11.6 -- not an asteroid (will add it to exclusion list)
06:44:38.40 -02:01:19.2 -- not an asteroid (will add it to exclusion list)
06:41:21.42 -00:35:22.3 -- not an asteroid (will add it to exclusion list)
06:48:12.25 -00:18:59.0 -- not an asteroid (will add it to exclusion list)
06:56:37.98 +00:11:23.8 -- not an asteroid (will add it to exclusion list)
06:49:55.03 -04:03:39.1 -- not an asteroid (will add it to exclusion list)
06:53:59.25 -01:54:57.4 -- not an asteroid (will add it to exclusion list)
06:55:12.13 +00:56:24.3 -- not an asteroid (will add it to exclusion list)
06:43:51.37 -04:55:44.4 -- not an asteroid (will add it to exclusion list)
06:55:50.86 -02:12:28.2 -- not an asteroid (will add it to exclusion list)
06:46:12.12 +00:43:13.7 -- not an asteroid (will add it to exclusion list)
06:53:08.29 -00:50:30.0 -- not an asteroid (will add it to exclusion list)
06:45:22.66 +01:37:11.2 -- not an asteroid (will add it to exclusion list)
06:51:39.84 -01:26:46.0 -- not an asteroid (will add it to exclusion list)
06:45:26.28 -00:11:50.6 -- not an asteroid (will add it to exclusion list)
06:47:53.26 +01:51:22.7 -- not an asteroid (will add it to exclusion list)
06:55:25.46 +00:38:48.5 -- not an asteroid (will add it to exclusion list)
06:52:15.24 -03:21:31.5 -- not an asteroid (will add it to exclusion list)
06:44:26.74 +00:04:54.9 -- not an asteroid (will add it to exclusion list)
06:51:33.88 -03:50:27.8 -- not an asteroid (will add it to exclusion list)
06:56:59.96 -00:24:06.2 -- not an asteroid (will add it to exclusion list)
06:47:10.04 -02:51:22.2 -- not an asteroid (will add it to exclusion list)
06:42:51.47 -04:30:08.4 -- not an asteroid (will add it to exclusion list)
06:41:26.98 -01:17:39.9 -- not an asteroid (will add it to exclusion list)
06:53:03.92 +01:25:47.9 -- not an asteroid (will add it to exclusion list)
06:52:31.95 -01:11:27.5 -- not an asteroid (will add it to exclusion list)
06:51:28.97 -01:28:26.1 -- not an asteroid (will add it to exclusion list)
06:51:21.48 +00:08:53.0 -- not an asteroid (will add it to exclusion list)
06:51:47.14 -01:07:36.4 -- not an asteroid (will add it to exclusion list)
06:50:21.65 -05:30:12.5 -- not an asteroid (will add it to exclusion list)
06:52:00.27 -01:37:37.6 -- not an asteroid (will add it to exclusion list)
06:55:33.00 +00:42:07.0 -- not an asteroid (will add it to exclusion list)
06:51:47.89 -00:51:42.9 -- not an asteroid (will add it to exclusion list)
06:52:19.95 +00:21:27.8 -- not an asteroid (will add it to exclusion list)
06:51:19.61 -01:48:26.6 -- not an asteroid (will add it to exclusion list)
06:54:08.45 +01:08:44.0 -- not an asteroid (will add it to exclusion list)
06:52:06.36 -01:18:21.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.51 -03:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:32.51 -03:35:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:58.68 -00:30:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:15.52 +00:55:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.26 -01:43:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.42 -00:35:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.98 -01:17:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.19 -01:19:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:58.95 -02:54:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:31.13 -06:04:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.31 -03:28:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:39.21 -02:16:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:51.47 -04:30:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.36 +01:58:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:22.36 +01:54:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:27.89 -03:56:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:37.06 -04:25:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:51.37 -04:55:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:55.64 -05:04:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:25.53 +01:06:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:26.10 +01:22:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:26.74 +00:04:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.17 -01:35:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:38.40 -02:01:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.62 -04:52:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.41 -00:01:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.72 +00:43:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:22.66 +01:37:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:26.28 -00:11:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.19 -00:09:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:12.12 +00:43:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:14.03 +00:50:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:19.49 -01:57:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.60 -00:28:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.08 +01:08:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.70 -01:51:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:42.50 -05:03:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:50.75 +01:18:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:09.69 -05:17:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.04 -02:51:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:12.07 +00:21:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:20.72 -05:40:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:53.26 +01:51:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:12.25 -00:18:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:21.59 +01:48:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:23.40 -05:30:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:34.77 -03:13:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:46.70 +01:42:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.53 -01:40:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:21.41 +01:13:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.51 -02:39:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:55.03 -04:03:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.12 -02:17:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:08.50 +00:46:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:14.58 -00:47:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.23 +00:24:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:21.65 -05:30:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:24.04 -01:20:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:34.46 -02:44:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.61 -00:31:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:54.65 -00:02:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.27 -01:42:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:19.61 -01:48:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:21.48 +00:08:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:22.49 +00:33:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:26.12 -01:48:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.97 -01:28:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.03 +00:27:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.88 -03:50:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.45 -01:39:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:39.84 -01:26:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:47.14 -01:07:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:47.89 -00:51:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:00.27 -01:37:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.36 -01:18:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:15.24 -03:21:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:19.95 +00:21:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:31.95 -01:11:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:34.75 +00:32:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:36.44 -02:12:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:55.21 -02:23:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:03.92 +01:25:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.25 -00:08:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.64 -05:33:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:08.29 -00:50:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:24.31 -05:41:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.93 -02:31:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.64 -00:33:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.72 -01:58:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.58 -02:38:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:50.88 -00:03:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.41 -02:12:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:59.25 -01:54:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:03.57 +02:06:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:08.45 +01:08:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:42.07 -02:41:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:43.94 -02:41:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:46.92 -00:18:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.61 +00:23:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:10.87 -00:02:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:10.99 -02:39:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:12.13 +00:56:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:16.14 +00:20:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:25.46 +00:38:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:27.37 -01:16:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:33.00 +00:42:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:37.02 -01:03:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:40.69 -00:18:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.86 -02:12:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:09.54 +00:41:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:11.81 -01:22:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:16.28 -01:49:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:17.34 +00:50:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:37.98 +00:11:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:38.45 -01:07:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.61 -01:04:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:59.96 -00:24:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.84 +00:55:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.50 +01:13:54.9 -- 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)
06:35:07.51 -03:03:03.8 -- not a known variable star
06:36:32.51 -03:35:54.2 -- not a known variable star
06:38:58.68 -00:30:12.9 -- not a known variable star
06:40:15.52 +00:55:17.2 -- a known variable star
06:41:21.26 -01:43:18.9 -- not a known variable star
06:41:21.42 -00:35:22.3 -- not a known variable star
06:41:26.98 -01:17:39.9 -- not a known variable star
06:41:27.19 -01:19:02.1 -- a known variable star
06:41:58.95 -02:54:56.4 -- not a known variable star
06:42:31.13 -06:04:20.9 -- a known variable star
06:42:33.31 -03:28:05.3 -- not a known variable star
06:42:39.21 -02:16:09.0 -- not a known variable star
06:42:51.47 -04:30:08.4 -- not a known variable star
06:43:14.36 +01:58:18.4 -- not a known variable star
06:43:22.36 +01:54:49.3 -- not a known variable star
06:43:27.89 -03:56:30.7 -- a known variable star
06:43:37.06 -04:25:01.6 -- a known variable star
06:43:51.37 -04:55:44.4 -- a known variable star
06:43:55.64 -05:04:02.0 -- not a known variable star
06:44:25.53 +01:06:41.9 -- not a known variable star
06:44:26.10 +01:22:07.5 -- not a known variable star
06:44:26.74 +00:04:54.9 -- not a known variable star
06:44:34.17 -01:35:28.4 -- a known variable star
06:44:38.40 -02:01:19.2 -- not a known variable star
06:44:50.62 -04:52:04.6 -- not a known variable star
06:45:12.41 -00:01:51.8 -- not a known variable star
06:45:17.72 +00:43:40.6 -- not a known variable star
06:45:22.66 +01:37:11.2 -- not a known variable star
06:45:26.28 -00:11:50.6 -- not a known variable star
06:45:54.19 -00:09:37.9 -- not a known variable star
06:46:12.12 +00:43:13.7 -- not a known variable star
06:46:14.03 +00:50:43.4 -- not a known variable star
06:46:19.49 -01:57:13.3 -- not a known variable star
06:46:25.60 -00:28:37.8 -- not a known variable star
06:46:31.08 +01:08:33.8 -- a known variable star
06:46:32.70 -01:51:11.6 -- not a known variable star
06:46:42.50 -05:03:51.9 -- not a known variable star
06:46:50.75 +01:18:08.1 -- a known variable star
06:47:09.69 -05:17:17.4 -- not a known variable star
06:47:10.04 -02:51:22.2 -- not a known variable star
06:47:12.07 +00:21:19.1 -- a known variable star
06:47:20.72 -05:40:15.0 -- a known variable star
06:47:53.26 +01:51:22.7 -- not a known variable star
06:48:12.25 -00:18:59.0 -- a known variable star
06:48:21.59 +01:48:28.8 -- not a known variable star
06:48:23.40 -05:30:23.9 -- not a known variable star
06:48:34.77 -03:13:30.5 -- not a known variable star
06:48:46.70 +01:42:52.1 -- not a known variable star
06:49:07.53 -01:40:18.1 -- not a known variable star
06:49:21.41 +01:13:45.9 -- not a known variable star
06:49:52.51 -02:39:52.3 -- not a known variable star
06:49:55.03 -04:03:39.1 -- not a known variable star
06:49:56.12 -02:17:03.6 -- not a known variable star
06:50:08.50 +00:46:16.9 -- a known variable star
06:50:14.58 -00:47:13.2 -- not a known variable star
06:50:18.23 +00:24:41.2 -- not a known variable star
06:50:21.65 -05:30:12.5 -- not a known variable star
06:50:24.04 -01:20:43.3 -- not a known variable star
06:50:34.46 -02:44:34.8 -- not a known variable star
06:50:41.61 -00:31:44.4 -- not a known variable star
06:50:54.65 -00:02:39.5 -- not a known variable star
06:51:10.27 -01:42:51.2 -- a known variable star
06:51:19.61 -01:48:26.6 -- not a known variable star
06:51:21.48 +00:08:53.0 -- not a known variable star
06:51:22.49 +00:33:44.7 -- not a known variable star
06:51:26.12 -01:48:02.1 -- not a known variable star
06:51:28.97 -01:28:26.1 -- not a known variable star
06:51:33.03 +00:27:11.8 -- a known variable star
06:51:33.88 -03:50:27.8 -- not a known variable star
06:51:34.45 -01:39:22.7 -- not a known variable star
06:51:39.84 -01:26:46.0 -- not a known variable star
06:51:47.14 -01:07:36.4 -- not a known variable star
06:51:47.89 -00:51:42.9 -- not a known variable star
06:52:00.27 -01:37:37.6 -- not a known variable star
06:52:06.36 -01:18:21.3 -- not a known variable star
06:52:15.24 -03:21:31.5 -- not a known variable star
06:52:19.95 +00:21:27.8 -- not a known variable star
06:52:31.95 -01:11:27.5 -- a known variable star
06:52:34.75 +00:32:33.5 -- not a known variable star
06:52:36.44 -02:12:52.8 -- not a known variable star
06:52:55.21 -02:23:01.3 -- not a known variable star
06:53:03.92 +01:25:47.9 -- not a known variable star
06:53:04.25 -00:08:10.5 -- a known variable star
06:53:04.64 -05:33:23.2 -- not a known variable star
06:53:08.29 -00:50:30.0 -- a known variable star
06:53:24.31 -05:41:34.5 -- a known variable star
06:53:36.93 -02:31:47.8 -- a known variable star
06:53:41.64 -00:33:48.7 -- a known variable star
06:53:43.72 -01:58:41.7 -- not a known variable star
06:53:47.58 -02:38:44.1 -- not a known variable star
06:53:50.88 -00:03:51.8 -- not a known variable star
06:53:52.41 -02:12:23.2 -- not a known variable star
06:53:59.25 -01:54:57.4 -- not a known variable star
06:54:03.57 +02:06:10.4 -- not a known variable star
06:54:08.45 +01:08:44.0 -- not a known variable star
06:54:42.07 -02:41:59.4 -- not a known variable star
06:54:43.94 -02:41:21.1 -- not a known variable star
06:54:46.92 -00:18:59.3 -- a known variable star
06:54:48.61 +00:23:18.5 -- a known variable star
06:55:10.87 -00:02:52.8 -- not a known variable star
06:55:10.99 -02:39:48.4 -- not a known variable star
06:55:12.13 +00:56:24.3 -- not a known variable star
06:55:16.14 +00:20:57.7 -- not a known variable star
06:55:25.46 +00:38:48.5 -- not a known variable star
06:55:27.37 -01:16:23.1 -- a known variable star
06:55:33.00 +00:42:07.0 -- not a known variable star
06:55:37.02 -01:03:22.4 -- a known variable star
06:55:40.69 -00:18:32.3 -- not a known variable star
06:55:50.86 -02:12:28.2 -- not a known variable star
06:56:09.54 +00:41:04.9 -- not a known variable star
06:56:11.81 -01:22:23.1 -- not a known variable star
06:56:16.28 -01:49:27.8 -- not a known variable star
06:56:17.34 +00:50:17.0 -- not a known variable star
06:56:37.98 +00:11:23.8 -- not a known variable star
06:56:38.45 -01:07:56.9 -- a known variable star
06:56:45.61 -01:04:28.3 -- not a known variable star
06:56:59.96 -00:24:06.2 -- not a known variable star
06:57:12.84 +00:55:21.6 -- not a known variable star
06:57:35.50 +01:13:54.9 -- a known variable star
Found 92 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
119 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 119 (excluding asteroids and hot pixels, 92 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461146.60882257 -observatory V36
00:07:51.35 -01:59:58.2 Mercury (0.0mag)
03:09:10.53 +17:53:55.3 Venus (-3.9mag)
00:18:08.96 +00:53:55.9 Mars (1.2mag)
07:12:40.81 +22:46:09.2 Jupiter (-2.1mag)
00:29:13.77 +00:49:17.0 Saturn (0.9mag)
03:47:43.19 +19:47:33.0 Uranus (5.8mag)
00:10:51.27 -00:15:16.9 Neptune (7.8mag)
20:33:45.55 -22:52:36.1 Pluto (14.5mag)
00:19:23.91 +04:31:23.4 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 361 Apr 15 22:11 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461146.60882257:
07:12:41.91 +22:46:09.4 Io (5.8mag)
07:12:46.08 +22:46:00.6 Europa (5.9mag)
07:12:57.89 +22:45:29.7 Ganymede (5.4mag)
07:13:16.19 +22:44:56.9 Callisto (6.6mag)
07:16:00.77 +22:33:43.7 Himalia (15.3mag)
07:12:39.31 +22:46:10.3 Thebe (16.2mag)
07:16:12.30 +23:03:55.8 Elara (17.3mag)
07:11:34.14 +23:26:06.2 Pasiphae (17.4mag)
07:21:00.37 +22:44:11.2 Carme (18.5mag)
00:29:14.34 +00:49:43.3 Titan (8.8mag)
00:29:12.21 +00:49:21.3 Rhea (10.1mag)
00:28:53.60 +00:49:25.4 Iapetus (11.5mag)
00:29:21.70 +00:49:37.1 Hyperion (14.8mag)
00:30:50.58 +00:58:04.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 15 22:11 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.60882257:
15:38:58.32 -16:18:41.1 JWST
13:11:27.65 +54:01:32.4 Chandra
07:50:49.45 -33:27:19.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 15 22:11 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.60882257 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:02.89 -28:47:06.7 13.9mag P/2010 H2 (Vales)
05:06:48.75 -69:39:24.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:28.16 +31:26:17.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:25.54 +10:33:38.0 17.6mag C/2021 G2 (ATLAS)
23:10:15.17 +29:13:59.4 17.1mag C/2022 E2 (ATLAS)
04:29:21.76 +26:02:29.3 16.0mag C/2022 N2 (PANSTARRS)
09:03:26.61 +32:01:06.3 16.2mag C/2022 QE78 (ATLAS)
08:31:05.39 -00:08:29.6 17.3mag C/2022 R6 (PANSTARRS)
18:53:42.37 +18:32:29.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:38.41 -11:31:12.0 17.5mag P/2023 B1 (PANSTARRS)
09:07:35.11 -11:51:56.6 17.6mag C/2023 F3 (ATLAS)
21:54:19.46 +62:54:45.4 17.5mag C/2023 H5 (Lemmon)
19:19:06.38 -03:44:03.3 14.1mag C/2023 R1 (PANSTARRS)
21:32:19.42 +85:55:34.9 17.8mag C/2023 X2 (Lemmon)
06:17:56.84 +63:30:45.4 17.2mag C/2024 A1 (ATLAS)
05:13:30.58 +18:20:41.4 11.1mag C/2024 E1 (Wierzchos)
16:19:12.44 +06:24:29.9 17.4mag C/2024 G6 (ATLAS)
20:20:50.54 +15:18:13.7 14.6mag C/2024 J3 (ATLAS)
03:26:27.92 -22:22:08.3 16.3mag C/2024 T5 (ATLAS)
05:16:48.25 +45:15:50.8 17.7mag C/2025 J1 (Borisov)
13:38:23.13 +45:33:43.1 15.2mag C/2025 L1 (ATLAS)
03:25:26.74 -26:13:43.4 17.8mag C/2025 Q3 (ATLAS)
23:44:21.37 +18:34:36.8 8.5mag C/2025 R3 (PANSTARRS)
12:54:04.31 +03:01:10.0 17.4mag C/2025 Y1 (ATLAS)
03:28:50.00 +02:36:30.0 13.3mag C/2026 A1 (MAPS)
23:59:53.29 +37:14:22.7 14.6mag C/2026 B2 (Sun-Gao)
18:43:08.79 -09:42:47.5 11.8mag 10P/Tempel
15:00:09.75 +03:11:53.1 14.0mag 24P/Schaumasse
11:02:46.42 -01:31:21.5 15.7mag 29P/Schwassmann-Wachmann
18:00:59.73 -09:36:21.7 17.9mag 40P/Vaisala
10:37:33.64 -04:05:24.6 16.9mag 43P/Wolf-Harrington
01:48:50.46 +17:30:22.5 17.2mag 47P/Ashbrook-Jackson
07:10:57.89 +36:59:23.0 17.0mag 63P/Wild
23:29:11.73 -11:26:15.9 15.7mag 65P/Gunn
04:03:32.29 +21:17:33.9 15.9mag 76P/West-Kohoutek-Ikemura
01:05:48.84 +08:15:00.5 14.3mag 78P/Gehrels
23:03:19.91 -09:21:32.2 14.6mag 88P/Howell
02:10:42.37 +20:40:17.6 15.1mag 93P/Lovas
04:55:00.43 +32:17:37.7 16.2mag 123P/West-Hartley
08:28:29.44 +38:18:40.3 16.2mag 124P/Mrkos
02:33:22.97 +14:22:56.0 16.4mag 128P/Shoemaker-Holt
02:47:44.98 +14:30:23.7 17.5mag 131P/Mueller
01:26:44.02 +13:16:35.3 10.6mag 141P/Machholz
01:35:38.90 +04:54:52.9 10.6mag 141P-A/Machholz
00:20:53.40 +00:49:11.5 12.8mag 141P-D/Machholz
02:05:59.19 +06:40:25.6 17.8mag 141P-I/Machholz
01:02:40.80 -01:28:15.9 15.1mag 162P/SidingSpring
14:51:14.53 -00:03:23.9 17.6mag 210P/Christensen
21:39:09.64 -11:25:20.2 17.6mag 218P/LINEAR
17:16:35.79 -13:55:12.2 16.1mag 235P/LINEAR
05:34:42.99 +34:42:26.8 16.8mag 240P/NEAT
07:38:32.82 -05:09:19.1 17.7mag 242P/Spahr
22:17:10.73 -20:57:04.1 17.9mag 260P/McNaught
01:58:24.60 +20:29:17.4 18.0mag 295P/LINEAR
15:42:36.29 +06:59:51.8 17.5mag 391P/Kowalski
07:34:14.24 +21:21:59.2 17.7mag 450P/LONEOS
05:36:01.73 +45:01:35.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 15 22:11 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 15 22:11 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:52:32.558 +54:28:28.21 AT 2026iyo 2026-04-07.50 19.8736
12:10:51.131 -15:24:05.80 AT 2026iyn 2026-04-07.49 19.8
10:03:32.464 +00:47:38.92 AT 2026iym 2026-04-09.07 21.7842
09:57:46.577 +02:32:54.17 AT 2026iyl 2026-04-09.07 21.1159
12:09:21.288 -14:20:40.69 AT 2026iyk 2026-02-24.42 19.0617
11:32:15.323 +26:34:23.97 AT 2026iyi 2026-04-07.27 20.0038
08:41:36.643 +41:14:51.53 AT 2026iyh 2026-03-18.28 20.5874
11:10:47.748 -02:27:00.61 AT 2026iyg 2026-04-07.26 20.12
11:41:25.329 -11:32:16.55 AT 2026iyf 2026-04-07.25 20.8489
09:58:35.594 -17:44:37.57 AT 2026iye 2026-04-08.19 19.4848
07:48:08.582 +43:35:35.35 AT 2026iyd 2026-04-05.16 19.8382
11:13:43.729 +21:50:31.84 AT 2026iyc 2026-04-05.18 20.0005
08:02:45.458 +40:40:22.73 AT 2026iyb 2026-03-26.18 20.4831
13:05:52.496 +64:22:32.75 AT 2026iya 2026-03-08.94 19.29
05:15:26.423 -02:54:24.54 AT 2026ixz 2026-04-08.14 19.1905
14:04:24.118 +43:40:15.80 AT 2026ixt 2026-04-08.93 19.74
13:12:41.279 +38:05:24.08 AT 2026ixs 2026-04-08.93 20.18
13:21:56.843 -04:01:33.33 AT 2026ixr 2026-04-08.90 19.48
12:04:52.343 +69:44:57.80 AT 2026ixq 2026-04-08.89 19.03
21:31:46.671 +04:33:36.35 AT 2026ixp 2026-04-08.51 19.1697
-rw-r--r-- 1 apache apache 30K Apr 15 22:11 tns_transients_list.txt
