This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461144.6113,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AG Mon 20260414.1113 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.4284-04.0114,2461144.6113,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.4284-04.0114 20260414.1113 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5329-01.2670,2461144.6113,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.5329-01.2670 20260414.1113 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,2461144.6113,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 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
ATO J104.8996+02.0661,2461144.6113,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8996+02.0661 20260414.1113 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119460486829616640,2461144.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119460486829616640 20260414.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6668-01.9250,2461144.6113,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6668-01.9250 20260414.1113 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107274358943072000,2461144.6113,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107274358943072000 20260414.1113 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4439-00.2500,2461144.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4439-00.2500 20260414.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 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 3120505602692442880,2461144.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120505602692442880 20260414.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.3925-03.5224,2461144.6113,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.3925-03.5224 20260414.1113 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
target,2461144.6113,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126395106665966080,2461144.6113,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126395106665966080 20260414.1113 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 J105.4876-02.6927,2461144.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.4876-02.6927 20260414.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5447+00.8442,2461144.6113,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.5447+00.8442 20260414.1113 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3060152756607968512,2461144.6113,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3060152756607968512 20260414.1113 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
target,2461144.6113,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9862+01.3992,2461144.6113,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9862+01.3992 20260414.1113 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114624353654375040,2461144.6113,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114624353654375040 20260414.1113 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107459557930729984,2461144.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107459557930729984 20260414.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070436.52+024443.7,2461144.6113,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070436.52+024443.7 20260414.1113 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0705000-020154,2461144.6113,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0705000-020154 20260414.1113 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112639799587138944,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112639799587138944 20260414.1113 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.43CV 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 3120794228792872960,2461144.6113,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120794228792872960 20260414.1113 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112750781541980032,2461144.6113,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112750781541980032 20260414.1113 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.43CV 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
ASASSN-V J064143.42-010627.5,2461144.6113,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064143.42-010627.5 20260414.1113 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059490751835095936,2461144.6113,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059490751835095936 20260414.1113 12.30CV 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 3059663100278940800,2461144.6113,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059663100278940800 20260414.1113 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0704125-011414,2461144.6113,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0704125-011414 20260414.1113 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059266687674749696,2461144.6113,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059266687674749696 20260414.1113 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125681313161965056,2461144.6113,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125681313161965056 20260414.1113 12.30CV 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 J098.7797-03.0546,2461144.6113,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260414.1113 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109471389332247552,2461144.6113,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109471389332247552 20260414.1113 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126260828808492544,2461144.6113,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126260828808492544 20260414.1113 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107964165049989376,2461144.6113,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107964165049989376 20260414.1113 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108464610338813696,2461144.6113,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108464610338813696 20260414.1113 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 14.1113 2461144.6113 12.02 07:06:54.61 -04:13:50.7
218.46193 1.50331 galactic Mon Second-epoch detections are separated by 0.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3107563977176844416 | 07:06:56.24 -04:13:48.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1949AnHar.112....1C HD 296299 J-Ks=0.073+/-0.041 (A)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3107563977176844416,2461144.6113,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3107563977176844416 20260414.1113 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.8979-01.9431,2461144.6113,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.8979-01.9431 20260414.1113 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12675437,2461144.6113,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12675437 20260414.1113 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108867959307360128,2461144.6113,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108867959307360128 20260414.1113 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115211321064418944,2461144.6113,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115211321064418944 20260414.1113 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7937+00.6981,2461144.6113,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7937+00.6981 20260414.1113 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059224670018297728,2461144.6113,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059224670018297728 20260414.1113 11.64CV 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 3101821880779349888,2461144.6113,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101821880779349888 20260414.1113 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
ATO J106.8650-01.8472,2461144.6113,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8650-01.8472 20260414.1113 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107635033119937152,2461144.6113,11.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107635033119937152 20260414.1113 11.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7472-02.9052,2461144.6113,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7472-02.9052 20260414.1113 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4169-01.4407,2461144.6113,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4169-01.4407 20260414.1113 11.14CV 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 J110.3037-02.2151,2461144.6113,11.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.3037-02.2151 20260414.1113 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822923819222400,2461144.6113,10.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822923819222400 20260414.1113 10.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1631+01.7787,2461144.6113,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260414.1113 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461144.6113,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260414.1113 11.43CV 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 3059411793155039360,2461144.6113,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059411793155039360 20260414.1113 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111447039926977152,2461144.6113,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111447039926977152 20260414.1113 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108508526385840000,2461144.6113,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108508526385840000 20260414.1113 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059953130831431680,2461144.6113,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059953130831431680 20260414.1113 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3121735956202275840,2461144.6113,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3121735956202275840 20260414.1113 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110277086535749248,2461144.6113,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110277086535749248 20260414.1113 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111755964035615104,2461144.6113,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111755964035615104 20260414.1113 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2433-00.4249,2461144.6113,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2433-00.4249 20260414.1113 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107244053654053376,2461144.6113,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107244053654053376 20260414.1113 12.03CV 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 3115503000884520448,2461144.6113,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115503000884520448 20260414.1113 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4987-02.8566,2461144.6113,12.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.4987-02.8566 20260414.1113 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119213405948991232,2461144.6113,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119213405948991232 20260414.1113 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1626-04.9704,2461144.6113,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1626-04.9704 20260414.1113 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119280785395344512,2461144.6113,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119280785395344512 20260414.1113 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.7366-03.4126,2461144.6113,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.7366-03.4126 20260414.1113 12.12CV 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 3114998496844392704,2461144.6113,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114998496844392704 20260414.1113 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7065-05.2541,2461144.6113,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7065-05.2541 20260414.1113 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059182270101246208,2461144.6113,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059182270101246208 20260414.1113 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113345346754410112,2461144.6113,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113345346754410112 20260414.1113 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2696-02.4769,2461144.6113,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2696-02.4769 20260414.1113 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.6697+03.0586,2461144.6113,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.6697+03.0586 20260414.1113 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100858296278549504,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100858296278549504 20260414.1113 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.6319-03.4457,2461144.6113,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.6319-03.4457 20260414.1113 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.37CV 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 3059651314888833408,2461144.6113,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059651314888833408 20260414.1113 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.43CV 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 3107717565213010816,2461144.6113,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107717565213010816 20260414.1113 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.0696-03.2272,2461144.6113,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.0696-03.2272 20260414.1113 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
target,2461144.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.43CV 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 3105965733946504448,2461144.6113,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105965733946504448 20260414.1113 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9551+00.2304,2461144.6113,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9551+00.2304 20260414.1113 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
target,2461144.6113,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8499-02.8303,2461144.6113,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8499-02.8303 20260414.1113 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 J109.0122+02.1631,2461144.6113,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.0122+02.1631 20260414.1113 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112749274012032640,2461144.6113,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112749274012032640 20260414.1113 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113610294697190784,2461144.6113,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113610294697190784 20260414.1113 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6113,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1113 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119467977252662016,2461144.6113,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119467977252662016 20260414.1113 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113103071939549184,2461144.6113,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113103071939549184 20260414.1113 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126439911764581760,2461144.6113,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126439911764581760 20260414.1113 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 J102.5828-06.4753,2461144.6113,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5828-06.4753 20260414.1113 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6933-02.7384,2461144.6113,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6933-02.7384 20260414.1113 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052748855768869760,2461144.6113,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3052748855768869760 20260414.1113 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105921684761121152,2461144.6113,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105921684761121152 20260414.1113 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461144.6113,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112424230887731712 20260414.1113 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111384127245493376,2461144.6113,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111384127245493376 20260414.1113 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1505+01.7467,2461144.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1505+01.7467 20260414.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105249642638290688,2461144.6113,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105249642638290688 20260414.1113 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127203655728648192,2461144.6113,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127203655728648192 20260414.1113 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17029,2461144.6113,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17029 20260414.1113 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461144.6113,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9913-01.3476 20260414.1113 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5594-03.0943,2461144.6113,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5594-03.0943 20260414.1113 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2108-02.3799,2461144.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2108-02.3799 20260414.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106128697885405184,2461144.6113,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106128697885405184 20260414.1113 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106985496621375104,2461144.6113,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106985496621375104 20260414.1113 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065110.72-012136.0,2461144.6113,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065110.72-012136.0 20260414.1113 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461144.6113,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BM Mon 20260414.1113 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461144.6113,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Mon 20260414.1113 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461144.61167671 14.04.2026 02:40:38.868 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
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): 34273
Objects passed selection criteria: 34145
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 26088
Average stars matched: 25295.8 (96.9632 %)
Memory usage VmPeak: 136940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:28:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461144.61167671 14.04.2026 02:40:38.868 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 310
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 128 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): 238143
Objects passed selection criteria: 237634
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: 196129
Average stars matched: 188788 (96.2573 %)
Memory usage VmPeak: 2051184 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:35:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.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: 2461144.61085134
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:20.707 -02:03:25.53
Angular distance between the image centers 0.1069 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:21.319 -02:04:06.48
Angular distance between the image centers 0.1108 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:20.707 -02:03:25.53
Second-epoch second image center 06:51:21.319 -02:04:06.48
Angular distance between the image centers 0.01166 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.pqdBqpwCyE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.BBY9byaNHD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.7uHlwq5aoz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits &> /tmp/tmp.LvmvONgeif
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.1 mag. fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
14.0 mag. fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.pqdBqpwCyE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BBY9byaNHD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.7uHlwq5aoz (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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1333, passed=16259
Got 16259 stars (including 14907 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 16259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 15985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 15984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 15984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 935 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LvmvONgeif (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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1305, passed=15771
Got 15771 stars (including 14443 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat
util/solve_plate_with_UCAC5 got 15771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 15453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out52823.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52823_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 52823_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53040_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 53040_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:48:24.51 -00:31:26.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.71 -02:21:30.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:20.707 -02:03:25.53
Angular distance between the image centers 0.1069 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:21.319 -02:04:06.48
Angular distance between the image centers 0.1108 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:20.707 -02:03:25.53
Second-epoch second image center 06:51:21.319 -02:04:06.48
Angular distance between the image centers 0.01166 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.9YFGPAKuq4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.63xjU5b7XM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits &> /tmp/tmp.dpDZ3goQla
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits &> /tmp/tmp.6LZlt6efNj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 296 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
2.0 pix fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.3 mag. fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
13.3 mag. fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.7 (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.9YFGPAKuq4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.63xjU5b7XM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dpDZ3goQla (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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=14991, passed=139402
Got 139402 stars (including 124237 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat
util/solve_plate_with_UCAC5 got 139402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 137754 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 137750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 137749 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6LZlt6efNj (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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=14317, passed=138018
Got 138018 stars (including 123513 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat
util/solve_plate_with_UCAC5 got 138018 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 136111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.8 to 3.7)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 136110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 136112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-39-27_20.00sec_-4.90C_LIGHTs_0030.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.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_2026-04-13_CI_Mon-02-Q1b1x1_214131_TTUQ1b1x1_15999_a6DlFI0R/wcs_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293053.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 157s
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: 85s
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Considering the candidate 288161_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288161_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:47:02.72 -03:47:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288163_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288163_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:06.45 -01:17:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.074 3112172545805041792 105.27769346465 -01.28925887652 14.1768 13.7202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288170_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288170_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288171_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288171_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288183_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288183_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288206_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288206_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288209_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288209_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:36:00.18 -01:43:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.946 3118793942263638400 099.00070840221 -01.72803940748 13.7274 13.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288217_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288217_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 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 288222_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288222_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288230_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288230_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288242_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288242_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:18:16.60 -01:57:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.178 3109767570279335296 109.56927424303 -01.95112301986 13.4672 13.0497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288244_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288244_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288248_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288248_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:49:14.21 +01:38:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288255_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288255_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:45.26 +02:52:16.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288256_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288256_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288257_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288257_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288263_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288263_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288264_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288264_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288265_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288265_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288266_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288266_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:40:52.90 -01:58:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288270_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288270_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288274_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288274_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288277_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288277_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:06:04.02 -00:02:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.105 3112734769903489536 106.51609385568 -00.03830975549 13.4506 12.6183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288278_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288278_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288280_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288280_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288281_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288281_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288287_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288287_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:05:19.29 -01:29:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.244 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288289_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288289_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:04:06.09 +02:29:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.393 3115593366996503296 106.02544925394 +02.49960695370 13.2839 12.2767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288302_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288302_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:46:18.27 +02:18:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.290 3126420773390408064 101.57604968922 +02.30161824287 13.6583 13.3169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288306_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288306_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288312_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288312_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:17:11.48 -00:21:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288315_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288315_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288316_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288316_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:16:07.24 +01:27:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288321_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288321_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:04:26.88 -07:12:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288323_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288323_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288326_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288326_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:28:29.54 +02:12:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288327_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288327_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:48:09.58 +03:04:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288328_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288328_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288333_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288333_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288335_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288335_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288336_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288336_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:19:04.48 -05:42:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288344_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:34:57.53 -03:16:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.874 3105103235793238656 098.73981880354 -03.26962395126 13.2415 12.6962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288345_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288345_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:06:26.57 +01:29:34.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288348_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288348_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:29.48 +02:40:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 3.399 3126318896766097664 103.62322431362 +02.67405695341 13.5130 13.0063 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288349_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288349_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288350_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288350_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:48:25.62 +02:36:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.432 3126458152488258944 102.10695934810 +02.60502436246 12.8136 11.6244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288354_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288354_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288356_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288356_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288357_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288357_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288358_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288358_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:54.72 +00:31:52.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288361_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288361_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288363_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288363_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288364_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288364_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288365_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288365_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:53:29.32 -06:31:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 4.112 3101010269399931392 103.37216687825 -06.52083675897 13.2056 12.7437 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288369_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288369_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:08:42.76 +01:59:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.737 3114730692744947456 107.17833101923 +01.99528879820 13.2190 12.4774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288371_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288371_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288372_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288372_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:46:12.53 +00:51:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288373_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288373_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:14:41.98 -01:47:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288375_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288375_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:02:01.39 -06:52:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.010 3052751570188346880 105.50594852052 -06.87284180315 13.2383 12.7040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288378_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288378_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288380_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288380_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:10:41.29 -05:05:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288383_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288383_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:03:27.03 -05:01:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288384_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288384_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:43.56 -02:48:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288385_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288385_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288386_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288386_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:18:36.22 -05:28:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288387_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288387_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288388_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288388_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:15:10.78 -00:43:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288394_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288394_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288401_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288401_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:16:00.23 +01:17:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.480 3111813211658797440 109.00189608583 +01.29951366799 13.0430 12.9505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288402_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288402_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288406_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288406_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:59:38.61 -06:13:04.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288407_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288407_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:17:17.39 -01:16:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288408_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288408_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288409_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288409_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:19:26.24 +01:43:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288410_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288410_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288414_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288414_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288418_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288418_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:42:09.68 -03:38:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.716 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288419_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288419_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:05:04.32 -05:27:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288421_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288421_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:05:11.14 -00:29:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.113 3112693400776779520 106.29629603399 -00.48935224730 12.8501 12.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288424_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288424_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288426_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288426_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:46:36.96 +02:52:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288428_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288428_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:52:13.32 -00:19:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288430_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288430_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:09.90 +01:52:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288431_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288431_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288435_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288435_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:08.18 -05:53:00.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 288436_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288436_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:19:17.21 -01:27:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288437_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288437_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:04:36.67 -01:40:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.136 3109456094950953344 106.15260396703 -01.66850726094 12.9200 12.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288438_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288438_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288440_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288440_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:21:33.45 -02:10:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288441_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288441_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:19:06.95 -06:36:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288442_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288442_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:41:45.12 -01:18:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288445_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288445_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:52:09.14 +00:34:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.175 3113585005929929984 103.03834255055 +00.57848204790 12.7509 11.9519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288450_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288450_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288452_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288452_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:03:52.74 +00:49:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.488 3114539549519264128 105.96987120849 +00.82965293709 12.7423 12.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288454_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288454_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:51:02.37 +01:07:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.102 3114047075689570688 102.75980879911 +01.12058532275 12.9570 12.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288455_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288455_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:33:59.85 +01:45:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 3.459 3120911322481431936 098.49950014419 +01.75665840777 12.7992 11.9050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288458_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288458_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288463_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:09:18.44 -01:42:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.312 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288464_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288464_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288466_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288466_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288470_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288470_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:13.81 -03:36:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 3.767 3102603805347108864 105.30706796189 -03.61185024820 12.7881 12.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288473_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288473_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:20:33.58 -04:55:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288475_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288475_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288479_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:21:17.54 -01:13:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288483_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288483_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:18:36.97 -05:27:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.609 3058400650470900864 109.65426555758 -05.45608185354 12.5828 11.8874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288487_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288487_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:44:38.77 -04:50:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.706 3103730014490289152 101.16173867769 -04.84495905347 12.3262 11.5571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288488_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288488_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288490_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288490_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:40.30 +01:01:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288494_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288494_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:19:17.57 +01:46:59.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288496_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288496_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288498_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288498_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:47:44.76 +02:19:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288499_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288499_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:18:50.90 -00:49:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288500_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288500_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288503_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288503_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:24.78 -01:42:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 2.851 3109118373080196224 105.35380665429 -01.71484121383 12.1150 11.6916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288505_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288505_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:16:02.27 -02:48:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288508_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288508_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:14:24.38 +01:15:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288512_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 288512_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288514_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288514_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:16:54.93 -06:19:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 8.60, MAG_FAINT_SEARCH_LIMIT=9.58)GAIADR2_OUTPUT=# 0.475 3058236891958149760 109.22900585891 -06.33191038881 9.5741 9.2658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288743_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 288743_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:20:21.10 -06:07:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.72, MAG_FAINT_SEARCH_LIMIT=10.70)GAIADR2_OUTPUT=# 0.786 3008152384963645184 095.08797473371 -06.12654381191 10.5149 10.2963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289224_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289224_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:14:38.85 -03:56:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289425_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289425_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:51:39.69 +00:25:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.230 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289471_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289471_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:46:13.05 +02:40:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289511_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289511_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:27:18.87 +00:20:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289683_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289683_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:44:27.32 +02:30:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.845 3127192557534558720 101.11392637967 +02.51524587168 12.3802 11.9793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289691_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289691_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:13:11.41 -02:19:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289745_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 289745_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289752_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 289752_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289798_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289798_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:02:11.21 -06:02:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.465 3053251431360757760 105.54685882342 -06.04380699213 12.3222 12.0281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289801_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289801_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:26:56.35 +00:49:08.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 289843_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 289843_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289854_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289854_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:33:06.31 +01:14:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 4.438 3120764095302536320 098.27668814582 +01.24558265169 12.4587 11.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289904_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289904_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:21:53.73 +02:20:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289920_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289920_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:50:41.56 -00:33:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289927_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289927_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:44:32.22 +03:08:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.007 3127298492907667840 101.13405560409 +03.14936616107 12.3190 11.4547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289949_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289949_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:09.41 -05:33:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289995_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 289995_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:36:41.09 -05:13:21.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290116_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290116_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290156_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290156_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:23:43.00 +02:39:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290166_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290166_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:21:54.65 +02:22:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290225_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290225_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:41:37.44 +03:12:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 2.367 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290249_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290249_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:16:32.80 -02:31:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290280_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290280_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:47:42.99 +02:23:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290288_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290288_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290370_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290370_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:22:45.48 -02:10:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290393_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290393_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:13:41.18 +00:46:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290397_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290397_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:21:45.61 +02:21:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290408_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290408_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290438_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290438_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:38:39.45 -01:31:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 3.893 3106905262331173632 099.66491829980 -01.52429610039 12.4571 11.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290449_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290449_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290456_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290456_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:24:43.19 -05:30:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290465_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290465_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:21:18.05 +02:01:28.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290479_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290479_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290482_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290482_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290489_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290489_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:58.66 -06:05:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.529 3101051771663735040 103.74453169028 -06.08582575552 12.6951 12.0997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290530_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290530_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:27:08.92 +00:16:36.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290552_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290552_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:47:19.65 +01:31:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.892 3125766220373632256 101.83212084767 +01.53059619715 12.9717 12.4642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290562_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290562_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:26:19.57 +01:23:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.014 3123455008273752704 096.58153352703 +01.38735719100 12.8884 12.3897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290568_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290568_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:52.65 -01:19:04.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290578_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290578_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:27:16.88 +02:55:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290602_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290602_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290616_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290616_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:14:03.88 -03:54:14.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290673_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290673_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290689_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290689_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290716_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290716_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290742_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290742_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:35:16.27 -04:45:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.338 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290748_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290748_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:37:58.41 -01:25:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.207 3118919183510887040 099.49400345973 -01.42388158330 12.8781 12.2501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290756_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290756_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290793_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290793_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:45:00.20 -00:03:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.657 3107483197430678400 101.25075565208 -00.05928951009 13.0563 12.7107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290809_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290809_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290847_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290847_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:05:01.46 +01:48:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.637 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290867_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290867_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:26:12.89 -01:34:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290869_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290869_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290871_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290871_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 290879_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290879_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:40:13.65 +01:34:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.336 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290882_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 290882_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 290886_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290886_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:22:49.92 -05:23:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290915_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290915_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:30.06 -04:07:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.617 3102509449203351296 103.62527411825 -04.12544889351 12.9516 12.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290920_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290920_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:49:33.80 -07:06:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290943_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290943_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:21:58.17 +00:11:01.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 290984_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290984_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:17:01.59 -02:44:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290987_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 290987_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:28:24.20 +02:02:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291008_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291008_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291031_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291031_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291033_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291033_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291036_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291036_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:31:44.88 -05:21:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291037_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291037_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 291092_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291092_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291094_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291094_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:13:58.92 -01:54:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291096_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291096_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291101_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291101_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:17:52.47 -07:05:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291114_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291114_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:02:39.62 -04:37:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.792 3101534633371804672 105.66529147356 -04.63116397367 12.8393 12.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291136_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291136_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:45.09 -07:09:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291158_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291158_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:09.47 -05:52:26.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291183_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291183_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291194_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291194_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:25:13.55 -00:55:32.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291208_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291208_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291224_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291224_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:45:04.75 -01:02:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291233_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291233_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:07:58.64 -00:56:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.951 3109605186152914432 106.99387176228 -00.94487186150 13.3450 12.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291252_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291252_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:22:26.70 -01:42:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.905 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291266_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291266_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:32:16.69 -00:38:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291291_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291291_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:32.35 -05:17:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 5.147 3101401244562695680 105.38457775638 -05.28896930257 12.4362 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291333_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291333_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:40:17.49 -04:25:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291346_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291346_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:43:09.44 -06:44:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291368_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291368_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:37:44.27 +02:40:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291371_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291371_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:56:45.69 +00:46:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.987 3113784979607011712 104.19017946265 +00.76807653068 13.3516 13.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291406_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291406_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291412_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291412_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291431_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291431_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:00:51.60 -03:52:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.999 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291442_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291442_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:22.90 +02:43:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291453_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291453_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:35.38 -02:56:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 4.090 3108133008808782208 108.14834035486 -02.93596888194 13.3637 12.6246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291455_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291455_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291459_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291459_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:40:18.97 +02:16:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.838 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291470_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291470_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:26:01.36 +01:41:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.708 3123897669081157248 096.50498777131 +01.69186981943 13.3939 12.8583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291488_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291488_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291496_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291496_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:34:14.95 -05:19:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291512_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291512_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:05:28.89 -01:00:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.591 3109568661751354496 106.37062191786 -01.00571634701 12.8404 11.9520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291513_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291513_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291518_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291518_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:47:26.24 +02:03:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.100 3126362769851744256 101.85924991798 +02.06333923017 13.2439 12.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291538_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291538_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:10:57.07 -04:52:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291539_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291539_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291578_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291578_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291593_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291593_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291613_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291613_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291653_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291653_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291664_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291664_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:06:30.37 -06:00:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291668_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291668_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 291672_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291672_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:53:58.21 -04:52:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291678_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291678_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291716_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291716_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:53:07.38 -01:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291745_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291745_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291759_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291759_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291760_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291760_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291770_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291770_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291771_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291771_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:22.76 -06:08:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.140 3052874406254774656 105.34484077065 -06.13892768243 13.2836 12.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291785_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291785_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:23.26 -01:37:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.234 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291832_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291832_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:44:26.18 -06:06:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.999 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291849_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291849_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:26:04.98 -04:38:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291868_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291868_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:02:19.65 -03:20:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.906 3108619920658643968 105.58111518078 -03.34490994692 13.4942 12.9329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291873_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291873_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:21:08.60 -06:35:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291882_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 291882_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 291895_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291895_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:49:10.59 -02:16:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291967_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291967_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:01:22.60 -03:06:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.636 3108642426286693376 105.34338227084 -03.10135969197 12.9086 11.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291973_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291973_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:08:43.12 -05:05:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291985_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291985_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:49:27.39 -07:09:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.023 3099371275519210496 102.36409163314 -07.15586692269 13.3778 12.9497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291991_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 291991_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:06:28.71 -05:58:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292027_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292042_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292042_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292052_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292052_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:00:53.31 +02:12:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.440 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292060_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292060_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292071_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292071_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:11:26.50 -01:03:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.106 3109380129868098176 107.86006082161 -01.05220251966 13.3067 12.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292076_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292076_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292092_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292092_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:32.84 -02:51:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292094_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292094_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:52:55.00 -02:23:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292127_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292127_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292129_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292129_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:32:41.66 +01:49:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292141_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292141_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:31:36.80 +00:48:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.941 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292156_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292156_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292190_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292190_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292214_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292214_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:24:01.94 -02:25:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292225_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292225_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292236_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292236_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:43:36.85 -04:25:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292248_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292248_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292270_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292270_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292304_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292304_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292315_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292315_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292357_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292357_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:43:50.45 +01:35:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.686 3125993196509475712 100.96104386401 +01.59687974744 13.5411 13.0702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292449_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292449_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:22:43.49 -02:10:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292499_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292499_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292505_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292505_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292533_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292533_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292554_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292554_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
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Considering the candidate 292615_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292615_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:29.65 -00:06:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292679_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292679_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292739_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292739_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:54:59.55 -01:03:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.927 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292844_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 292844_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292847_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292847_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:53.93 +01:22:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292872_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 292872_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:06:37.12 -04:38:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.098 3101496459701712640 106.65476195883 -04.63532880131 13.6813 13.0848 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293003_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 293003_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293053_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 293053_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293087_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 293087_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:44:50.41 +01:05:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.137 3125637783672257024 101.21022796390 +01.09398203346 14.0648 13.6219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 121122_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:09:13.64 -02:21:30.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 65114_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:27:01.26 -04:35:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91187_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 91187_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:29:53.90 -03:35:06.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 06:50:00.66 +01:46:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.097 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031 did not pass the final checks
**** FOUND 07:12:52.05 -05:20:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-13_21-40-38_20.00sec_-4.90C_LIGHTs_0031
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 248s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.71 -02:21:30.7
07:08:45.30 +00:41:47.8
07:17:30.87 +01:05:34.5
06:57:42.55 -04:00:45.5
06:58:09.31 -01:15:58.8
06:39:50.61 +00:48:18.6
06:50:23.99 -01:20:42.3
06:59:34.41 +02:03:39.0
06:42:40.69 -00:18:16.1
06:58:39.23 -01:55:06.6
06:40:43.55 -01:24:10.0
06:53:46.02 -00:14:35.2
06:59:29.48 +02:30:33.3
07:00:09.60 -00:53:36.6
07:07:24.30 +02:31:24.7
06:32:24.05 +00:26:60.0
07:13:31.49 -03:31:14.5
06:40:41.57 +01:46:32.9
07:00:51.57 +01:33:15.9
06:49:52.98 +02:30:13.8
07:01:56.24 -02:41:24.4
06:46:13.81 +00:50:43.9
07:17:33.93 -02:54:19.7
07:06:06.05 -05:15:50.3
06:43:56.11 +01:24:34.9
07:03:11.48 +01:23:09.8
06:46:00.36 -00:22:09.4
07:04:35.22 +02:44:56.4
07:05:00.36 -02:02:17.7
06:59:40.23 -00:39:47.2
07:22:14.40 -00:18:40.7
06:30:06.27 +01:09:03.2
06:56:42.67 +02:46:48.5
07:05:15.60 +00:02:29.2
06:39:28.64 -05:35:45.9
07:09:57.98 +00:39:41.7
06:41:43.24 -01:05:57.7
07:10:37.57 -04:15:16.6
07:18:56.39 -04:19:24.8
07:04:11.71 -01:14:18.4
07:17:04.21 -04:46:11.1
06:49:22.84 +01:06:39.0
06:35:07.42 -03:03:04.8
07:05:18.16 -01:22:58.4
07:13:32.91 +00:13:00.8
06:53:55.08 +02:25:33.0
07:07:58.87 -02:58:38.3
07:09:57.25 -01:59:05.8
07:06:54.61 -04:13:50.7
07:19:35.86 -01:56:19.0
07:18:41.90 +01:11:03.4
07:05:50.95 -02:05:12.3
07:09:20.59 +02:38:44.5
06:59:09.68 +00:41:52.9
07:16:33.92 -05:05:59.1
07:02:21.48 -04:03:29.9
07:07:26.04 -01:50:45.3
07:10:59.18 -03:55:09.2
07:11:00.56 -02:53:39.2
07:09:43.85 -01:26:40.3
07:21:14.19 -02:12:39.7
07:17:51.14 -01:41:37.5
07:08:35.58 +01:46:44.9
06:40:30.45 -01:04:41.2
07:11:05.25 -04:42:12.3
07:17:52.75 +00:17:04.1
07:14:13.13 -01:59:27.9
07:17:39.07 -03:44:22.0
06:21:17.05 -00:11:56.5
07:19:20.14 -00:18:59.1
07:17:38.05 +01:13:00.8
07:01:00.94 -00:25:43.7
06:43:35.22 -01:19:39.7
07:01:21.72 +02:15:51.4
07:14:00.00 -02:51:46.9
06:35:26.35 -00:39:36.8
07:04:39.04 -04:57:05.5
06:34:11.05 -00:21:49.2
07:20:04.04 +02:27:50.8
06:22:56.71 -03:24:45.7
07:17:13.72 +02:22:35.4
06:56:45.12 +00:46:35.9
07:18:50.05 -05:15:16.6
07:13:04.72 -05:12:24.0
06:51:28.85 -00:00:28.7
07:09:03.33 -02:29:06.4
06:34:40.00 +03:03:22.1
06:55:38.92 -06:15:20.8
06:44:31.46 +00:07:35.0
07:02:30.67 -03:26:39.2
06:45:06.13 -00:02:48.1
07:18:20.69 -04:33:00.2
06:43:32.18 -01:20:34.7
07:08:08.39 -03:34:58.8
06:44:16.55 -03:13:34.6
06:49:44.06 -06:16:27.3
06:53:36.78 -02:31:44.3
06:47:47.43 +00:13:39.7
06:40:19.77 -03:22:49.5
07:03:23.99 -02:49:51.6
07:16:03.90 +02:09:51.0
07:05:14.71 +00:02:16.2
06:48:48.39 +00:23:30.8
07:20:04.65 +02:28:16.8
06:41:47.09 -00:16:14.5
07:01:14.48 +00:57:27.9
06:46:37.29 +02:26:40.4
06:50:19.49 -06:27:50.5
06:42:46.39 -02:44:16.6
07:03:07.68 -06:51:54.1
06:49:56.23 -02:40:55.1
06:56:21.96 -00:53:11.0
07:11:54.51 +00:45:39.1
06:44:35.73 +01:45:23.6
06:44:17.33 -04:35:49.7
06:45:39.07 +02:45:24.8
06:40:33.81 -03:31:37.1
06:47:59.52 -01:20:54.6
07:02:14.49 -03:05:56.6
06:52:51.70 -02:22:43.9
06:49:56.01 -02:17:06.0
06:46:51.83 -01:38:32.2
06:51:10.70 -01:21:35.2
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:09:13.71 -02:21:30.7
06:57:42.55 -04:00:45.5
06:58:09.31 -01:15:58.8
06:39:50.61 +00:48:18.6
06:50:23.99 -01:20:42.3
06:59:34.41 +02:03:39.0
06:42:40.69 -00:18:16.1
06:58:39.23 -01:55:06.6
06:40:43.55 -01:24:10.0
06:53:46.02 -00:14:35.2
06:59:29.48 +02:30:33.3
07:00:09.60 -00:53:36.6
07:07:24.30 +02:31:24.7
06:32:24.05 +00:26:60.0
07:13:31.49 -03:31:14.5
06:40:41.57 +01:46:32.9
07:00:51.57 +01:33:15.9
06:49:52.98 +02:30:13.8
07:01:56.24 -02:41:24.4
06:46:13.81 +00:50:43.9
07:17:33.93 -02:54:19.7
07:06:06.05 -05:15:50.3
06:43:56.11 +01:24:34.9
07:03:11.48 +01:23:09.8
06:46:00.36 -00:22:09.4
07:04:35.22 +02:44:56.4
07:05:00.36 -02:02:17.7
06:59:40.23 -00:39:47.2
07:22:14.40 -00:18:40.7
06:30:06.27 +01:09:03.2
06:56:42.67 +02:46:48.5
07:05:15.60 +00:02:29.2
06:39:28.64 -05:35:45.9
07:09:57.98 +00:39:41.7
06:41:43.24 -01:05:57.7
07:10:37.57 -04:15:16.6
07:18:56.39 -04:19:24.8
07:04:11.71 -01:14:18.4
07:17:04.21 -04:46:11.1
06:49:22.84 +01:06:39.0
06:35:07.42 -03:03:04.8
07:05:18.16 -01:22:58.4
07:13:32.91 +00:13:00.8
06:53:55.08 +02:25:33.0
07:07:58.87 -02:58:38.3
07:09:57.25 -01:59:05.8
07:06:54.61 -04:13:50.7
07:19:35.86 -01:56:19.0
07:18:41.90 +01:11:03.4
07:05:50.95 -02:05:12.3
07:09:20.59 +02:38:44.5
06:59:09.68 +00:41:52.9
07:16:33.92 -05:05:59.1
07:02:21.48 -04:03:29.9
07:07:26.04 -01:50:45.3
07:10:59.18 -03:55:09.2
07:11:00.56 -02:53:39.2
07:09:43.85 -01:26:40.3
07:21:14.19 -02:12:39.7
07:17:51.14 -01:41:37.5
07:08:35.58 +01:46:44.9
06:40:30.45 -01:04:41.2
07:11:05.25 -04:42:12.3
07:17:52.75 +00:17:04.1
07:14:13.13 -01:59:27.9
07:17:39.07 -03:44:22.0
06:21:17.05 -00:11:56.5
07:19:20.14 -00:18:59.1
07:17:38.05 +01:13:00.8
07:01:00.94 -00:25:43.7
06:43:35.22 -01:19:39.7
07:01:21.72 +02:15:51.4
07:14:00.00 -02:51:46.9
06:35:26.35 -00:39:36.8
07:04:39.04 -04:57:05.5
06:34:11.05 -00:21:49.2
07:20:04.04 +02:27:50.8
06:22:56.71 -03:24:45.7
07:17:13.72 +02:22:35.4
06:56:45.12 +00:46:35.9
07:18:50.05 -05:15:16.6
07:13:04.72 -05:12:24.0
06:51:28.85 -00:00:28.7
07:09:03.33 -02:29:06.4
06:34:40.00 +03:03:22.1
06:55:38.92 -06:15:20.8
06:44:31.46 +00:07:35.0
07:02:30.67 -03:26:39.2
06:45:06.13 -00:02:48.1
07:18:20.69 -04:33:00.2
06:43:32.18 -01:20:34.7
07:08:08.39 -03:34:58.8
06:44:16.55 -03:13:34.6
06:49:44.06 -06:16:27.3
06:53:36.78 -02:31:44.3
06:47:47.43 +00:13:39.7
06:40:19.77 -03:22:49.5
07:03:23.99 -02:49:51.6
07:16:03.90 +02:09:51.0
07:05:14.71 +00:02:16.2
06:48:48.39 +00:23:30.8
07:20:04.65 +02:28:16.8
06:41:47.09 -00:16:14.5
07:01:14.48 +00:57:27.9
06:46:37.29 +02:26:40.4
06:50:19.49 -06:27:50.5
06:42:46.39 -02:44:16.6
07:03:07.68 -06:51:54.1
06:49:56.23 -02:40:55.1
06:56:21.96 -00:53:11.0
07:11:54.51 +00:45:39.1
06:44:35.73 +01:45:23.6
06:44:17.33 -04:35:49.7
06:45:39.07 +02:45:24.8
06:40:33.81 -03:31:37.1
06:47:59.52 -01:20:54.6
07:02:14.49 -03:05:56.6
06:52:51.70 -02:22:43.9
06:49:56.01 -02:17:06.0
06:46:51.83 -01:38:32.2
06:51:10.70 -01:21:35.2
07:08:45.30 +00:41:47.8
07:17:30.87 +01:05:34.5
###################################################################################
07:09:13.71 -02:21:30.7 -- not an asteroid (will add it to exclusion list)
06:57:42.55 -04:00:45.5 -- not an asteroid (will add it to exclusion list)
06:58:09.31 -01:15:58.8 -- not an asteroid (will add it to exclusion list)
06:39:50.61 +00:48:18.6 -- not an asteroid (will add it to exclusion list)
06:50:23.99 -01:20:42.3 -- not an asteroid (will add it to exclusion list)
06:59:34.41 +02:03:39.0 -- not an asteroid (will add it to exclusion list)
06:42:40.69 -00:18:16.1 -- not an asteroid (will add it to exclusion list)
06:58:39.23 -01:55:06.6 -- not an asteroid (will add it to exclusion list)
06:40:43.55 -01:24:10.0 -- not an asteroid (will add it to exclusion list)
06:53:46.02 -00:14:35.2 -- not an asteroid (will add it to exclusion list)
06:59:29.48 +02:30:33.3 -- not an asteroid (will add it to exclusion list)
07:00:09.60 -00:53:36.6 -- not an asteroid (will add it to exclusion list)
07:07:24.30 +02:31:24.7 -- not an asteroid (will add it to exclusion list)
06:32:24.05 +00:26:60.0 -- not an asteroid (will add it to exclusion list)
07:13:31.49 -03:31:14.5 -- not an asteroid (will add it to exclusion list)
06:40:41.57 +01:46:32.9 -- not an asteroid (will add it to exclusion list)
07:00:51.57 +01:33:15.9 -- not an asteroid (will add it to exclusion list)
06:49:52.98 +02:30:13.8 -- not an asteroid (will add it to exclusion list)
07:01:56.24 -02:41:24.4 -- not an asteroid (will add it to exclusion list)
06:46:13.81 +00:50:43.9 -- not an asteroid (will add it to exclusion list)
07:17:33.93 -02:54:19.7 -- not an asteroid (will add it to exclusion list)
07:06:06.05 -05:15:50.3 -- not an asteroid (will add it to exclusion list)
06:43:56.11 +01:24:34.9 -- not an asteroid (will add it to exclusion list)
07:03:11.48 +01:23:09.8 -- not an asteroid (will add it to exclusion list)
06:46:00.36 -00:22:09.4 -- not an asteroid (will add it to exclusion list)
07:04:35.22 +02:44:56.4 -- not an asteroid (will add it to exclusion list)
07:05:00.36 -02:02:17.7 -- not an asteroid (will add it to exclusion list)
06:59:40.23 -00:39:47.2 -- not an asteroid (will add it to exclusion list)
07:22:14.40 -00:18:40.7 -- not an asteroid (will add it to exclusion list)
06:30:06.27 +01:09:03.2 -- not an asteroid (will add it to exclusion list)
06:56:42.67 +02:46:48.5 -- not an asteroid (will add it to exclusion list)
07:05:15.60 +00:02:29.2 -- not an asteroid (will add it to exclusion list)
06:39:28.64 -05:35:45.9 -- not an asteroid (will add it to exclusion list)
07:09:57.98 +00:39:41.7 -- not an asteroid (will add it to exclusion list)
06:41:43.24 -01:05:57.7 -- not an asteroid (will add it to exclusion list)
07:10:37.57 -04:15:16.6 -- not an asteroid (will add it to exclusion list)
07:18:56.39 -04:19:24.8 -- not an asteroid (will add it to exclusion list)
07:04:11.71 -01:14:18.4 -- not an asteroid (will add it to exclusion list)
07:17:04.21 -04:46:11.1 -- not an asteroid (will add it to exclusion list)
06:49:22.84 +01:06:39.0 -- not an asteroid (will add it to exclusion list)
06:35:07.42 -03:03:04.8 -- not an asteroid (will add it to exclusion list)
07:05:18.16 -01:22:58.4 -- not an asteroid (will add it to exclusion list)
07:13:32.91 +00:13:00.8 -- not an asteroid (will add it to exclusion list)
06:53:55.08 +02:25:33.0 -- not an asteroid (will add it to exclusion list)
07:07:58.87 -02:58:38.3 -- not an asteroid (will add it to exclusion list)
07:09:57.25 -01:59:05.8 -- not an asteroid (will add it to exclusion list)
07:06:54.61 -04:13:50.7 -- not an asteroid (will add it to exclusion list)
07:19:35.86 -01:56:19.0 -- not an asteroid (will add it to exclusion list)
07:18:41.90 +01:11:03.4 -- not an asteroid (will add it to exclusion list)
07:05:50.95 -02:05:12.3 -- not an asteroid (will add it to exclusion list)
07:09:20.59 +02:38:44.5 -- not an asteroid (will add it to exclusion list)
06:59:09.68 +00:41:52.9 -- not an asteroid (will add it to exclusion list)
07:16:33.92 -05:05:59.1 -- not an asteroid (will add it to exclusion list)
07:02:21.48 -04:03:29.9 -- not an asteroid (will add it to exclusion list)
07:07:26.04 -01:50:45.3 -- not an asteroid (will add it to exclusion list)
07:10:59.18 -03:55:09.2 -- not an asteroid (will add it to exclusion list)
07:11:00.56 -02:53:39.2 -- not an asteroid (will add it to exclusion list)
07:09:43.85 -01:26:40.3 -- not an asteroid (will add it to exclusion list)
07:21:14.19 -02:12:39.7 -- not an asteroid (will add it to exclusion list)
07:17:51.14 -01:41:37.5 -- not an asteroid (will add it to exclusion list)
07:08:35.58 +01:46:44.9 -- not an asteroid (will add it to exclusion list)
06:40:30.45 -01:04:41.2 -- not an asteroid (will add it to exclusion list)
07:11:05.25 -04:42:12.3 -- not an asteroid (will add it to exclusion list)
07:17:52.75 +00:17:04.1 -- not an asteroid (will add it to exclusion list)
07:14:13.13 -01:59:27.9 -- not an asteroid (will add it to exclusion list)
07:17:39.07 -03:44:22.0 -- not an asteroid (will add it to exclusion list)
06:21:17.05 -00:11:56.5 -- not an asteroid (will add it to exclusion list)
07:19:20.14 -00:18:59.1 -- not an asteroid (will add it to exclusion list)
07:17:38.05 +01:13:00.8 -- not an asteroid (will add it to exclusion list)
07:01:00.94 -00:25:43.7 -- not an asteroid (will add it to exclusion list)
06:43:35.22 -01:19:39.7 -- not an asteroid (will add it to exclusion list)
07:01:21.72 +02:15:51.4 -- not an asteroid (will add it to exclusion list)
07:14:00.00 -02:51:46.9 -- not an asteroid (will add it to exclusion list)
06:35:26.35 -00:39:36.8 -- not an asteroid (will add it to exclusion list)
07:04:39.04 -04:57:05.5 -- not an asteroid (will add it to exclusion list)
06:34:11.05 -00:21:49.2 -- not an asteroid (will add it to exclusion list)
07:20:04.04 +02:27:50.8 -- not an asteroid (will add it to exclusion list)
06:22:56.71 -03:24:45.7 -- not an asteroid (will add it to exclusion list)
07:17:13.72 +02:22:35.4 -- not an asteroid (will add it to exclusion list)
06:56:45.12 +00:46:35.9 -- not an asteroid (will add it to exclusion list)
07:18:50.05 -05:15:16.6 -- not an asteroid (will add it to exclusion list)
07:13:04.72 -05:12:24.0 -- not an asteroid (will add it to exclusion list)
06:51:28.85 -00:00:28.7 -- not an asteroid (will add it to exclusion list)
07:09:03.33 -02:29:06.4 -- not an asteroid (will add it to exclusion list)
06:34:40.00 +03:03:22.1 -- not an asteroid (will add it to exclusion list)
06:55:38.92 -06:15:20.8 -- not an asteroid (will add it to exclusion list)
06:44:31.46 +00:07:35.0 -- not an asteroid (will add it to exclusion list)
07:02:30.67 -03:26:39.2 -- not an asteroid (will add it to exclusion list)
06:45:06.13 -00:02:48.1 -- not an asteroid (will add it to exclusion list)
07:18:20.69 -04:33:00.2 -- not an asteroid (will add it to exclusion list)
06:43:32.18 -01:20:34.7 -- not an asteroid (will add it to exclusion list)
07:08:08.39 -03:34:58.8 -- not an asteroid (will add it to exclusion list)
06:44:16.55 -03:13:34.6 -- not an asteroid (will add it to exclusion list)
06:49:44.06 -06:16:27.3 -- not an asteroid (will add it to exclusion list)
06:53:36.78 -02:31:44.3 -- not an asteroid (will add it to exclusion list)
06:47:47.43 +00:13:39.7 -- not an asteroid (will add it to exclusion list)
06:40:19.77 -03:22:49.5 -- not an asteroid (will add it to exclusion list)
07:03:23.99 -02:49:51.6 -- not an asteroid (will add it to exclusion list)
07:16:03.90 +02:09:51.0 -- not an asteroid (will add it to exclusion list)
07:05:14.71 +00:02:16.2 -- not an asteroid (will add it to exclusion list)
06:48:48.39 +00:23:30.8 -- not an asteroid (will add it to exclusion list)
07:20:04.65 +02:28:16.8 -- not an asteroid (will add it to exclusion list)
06:41:47.09 -00:16:14.5 -- not an asteroid (will add it to exclusion list)
07:01:14.48 +00:57:27.9 -- not an asteroid (will add it to exclusion list)
06:46:37.29 +02:26:40.4 -- not an asteroid (will add it to exclusion list)
06:50:19.49 -06:27:50.5 -- not an asteroid (will add it to exclusion list)
06:42:46.39 -02:44:16.6 -- not an asteroid (will add it to exclusion list)
07:03:07.68 -06:51:54.1 -- not an asteroid (will add it to exclusion list)
06:49:56.23 -02:40:55.1 -- not an asteroid (will add it to exclusion list)
06:56:21.96 -00:53:11.0 -- not an asteroid (will add it to exclusion list)
07:11:54.51 +00:45:39.1 -- not an asteroid (will add it to exclusion list)
06:44:35.73 +01:45:23.6 -- not an asteroid (will add it to exclusion list)
06:44:17.33 -04:35:49.7 -- not an asteroid (will add it to exclusion list)
06:45:39.07 +02:45:24.8 -- not an asteroid (will add it to exclusion list)
06:40:33.81 -03:31:37.1 -- not an asteroid (will add it to exclusion list)
06:47:59.52 -01:20:54.6 -- not an asteroid (will add it to exclusion list)
07:02:14.49 -03:05:56.6 -- not an asteroid (will add it to exclusion list)
06:52:51.70 -02:22:43.9 -- not an asteroid (will add it to exclusion list)
06:49:56.01 -02:17:06.0 -- not an asteroid (will add it to exclusion list)
06:46:51.83 -01:38:32.2 -- not an asteroid (will add it to exclusion list)
06:51:10.70 -01:21:35.2 -- not an asteroid (will add it to exclusion list)
07:08:45.30 +00:41:47.8 -- not an asteroid (will add it to exclusion list)
07:17:30.87 +01:05:34.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:21:17.05 -00:11:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:56.71 -03:24:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:06.27 +01:09:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:24.05 +00:26:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:11.05 -00:21:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:40.00 +03:03:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:07.42 -03:03:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:26.35 -00:39:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:28.64 -05:35:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:50.61 +00:48:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:19.77 -03:22:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.45 -01:04:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:33.81 -03:31:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:41.57 +01:46:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:43.55 -01:24:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:43.24 -01:05:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:47.09 -00:16:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:40.69 -00:18:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:46.39 -02:44:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:32.18 -01:20:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:35.22 -01:19:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:56.11 +01:24:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:16.55 -03:13:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:17.33 -04:35:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.46 +00:07:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:35.73 +01:45:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:06.13 -00:02:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.07 +02:45:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:00.36 -00:22:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.81 +00:50:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:37.29 +02:26:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:51.83 -01:38:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:47.43 +00:13:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.52 -01:20:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:48.39 +00:23:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:22.84 +01:06:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:44.06 -06:16:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.98 +02:30:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.01 -02:17:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.23 -02:40:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:19.49 -06:27:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:23.99 -01:20:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.70 -01:21:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.85 -00:00:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.70 -02:22:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.78 -02:31:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:46.02 -00:14:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:55.08 +02:25:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:38.92 -06:15:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:21.96 -00:53:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:42.67 +02:46:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.12 +00:46:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:42.55 -04:00:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:09.31 -01:15:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.23 -01:55:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:09.68 +00:41:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:29.48 +02:30:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:34.41 +02:03:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:40.23 -00:39:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:09.60 -00:53:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.57 +01:33:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.94 -00:25:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.48 +00:57:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:21.72 +02:15:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:56.24 -02:41:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.49 -03:05:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.48 -04:03:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:30.67 -03:26:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:07.68 -06:51:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:11.48 +01:23:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:23.99 -02:49:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:11.71 -01:14:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:35.22 +02:44:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:39.04 -04:57:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:00.36 -02:02:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.71 +00:02:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:15.60 +00:02:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.16 -01:22:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.95 -02:05:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:06.05 -05:15:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.61 -04:13:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.30 +02:31:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.04 -01:50:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:58.87 -02:58:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:08.39 -03:34:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.58 +01:46:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.30 +00:41:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:03.33 -02:29:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.71 -02:21:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.59 +02:38:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:43.85 -01:26:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:57.25 -01:59:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:57.98 +00:39:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:37.57 -04:15:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:59.18 -03:55:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:00.56 -02:53:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:05.25 -04:42:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:54.51 +00:45:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:04.72 -05:12:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:31.49 -03:31:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:32.91 +00:13:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:00.00 -02:51:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:13.13 -01:59:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.90 +02:09:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:33.92 -05:05:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:04.21 -04:46:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:13.72 +02:22:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:30.87 +01:05:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:33.93 -02:54:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:38.05 +01:13:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:39.07 -03:44:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:51.14 -01:41:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:52.75 +00:17:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:20.69 -04:33:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:41.90 +01:11:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:50.05 -05:15:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:56.39 -04:19:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:20.14 -00:18:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:35.86 -01:56:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:04.04 +02:27:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:04.65 +02:28:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:14.19 -02:12:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:14.40 -00:18:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:21:17.05 -00:11:56.5 -- not a known variable star
06:22:56.71 -03:24:45.7 -- not a known variable star
06:30:06.27 +01:09:03.2 -- a known variable star
06:32:24.05 +00:26:60.0 -- not a known variable star
06:34:11.05 -00:21:49.2 -- not a known variable star
06:34:40.00 +03:03:22.1 -- not a known variable star
06:35:07.42 -03:03:04.8 -- not a known variable star
06:35:26.35 -00:39:36.8 -- not a known variable star
06:39:28.64 -05:35:45.9 -- not a known variable star
06:39:50.61 +00:48:18.6 -- not a known variable star
06:40:19.77 -03:22:49.5 -- not a known variable star
06:40:30.45 -01:04:41.2 -- a known variable star
06:40:33.81 -03:31:37.1 -- not a known variable star
06:40:41.57 +01:46:32.9 -- not a known variable star
06:40:43.55 -01:24:10.0 -- a known variable star
06:41:43.24 -01:05:57.7 -- not a known variable star
06:41:47.09 -00:16:14.5 -- not a known variable star
06:42:40.69 -00:18:16.1 -- a known variable star
06:42:46.39 -02:44:16.6 -- not a known variable star
06:43:32.18 -01:20:34.7 -- not a known variable star
06:43:35.22 -01:19:39.7 -- a known variable star
06:43:56.11 +01:24:34.9 -- not a known variable star
06:44:16.55 -03:13:34.6 -- not a known variable star
06:44:17.33 -04:35:49.7 -- a known variable star
06:44:31.46 +00:07:35.0 -- not a known variable star
06:44:35.73 +01:45:23.6 -- not a known variable star
06:45:06.13 -00:02:48.1 -- not a known variable star
06:45:39.07 +02:45:24.8 -- a known variable star
06:46:00.36 -00:22:09.4 -- not a known variable star
06:46:13.81 +00:50:43.9 -- not a known variable star
06:46:37.29 +02:26:40.4 -- not a known variable star
06:46:51.83 -01:38:32.2 -- not a known variable star
06:47:47.43 +00:13:39.7 -- not a known variable star
06:47:59.52 -01:20:54.6 -- not a known variable star
06:48:48.39 +00:23:30.8 -- a known variable star
06:49:22.84 +01:06:39.0 -- a known variable star
06:49:44.06 -06:16:27.3 -- not a known variable star
06:49:52.98 +02:30:13.8 -- a known variable star
06:49:56.01 -02:17:06.0 -- not a known variable star
06:49:56.23 -02:40:55.1 -- not a known variable star
06:50:19.49 -06:27:50.5 -- not a known variable star
06:50:23.99 -01:20:42.3 -- not a known variable star
06:51:10.70 -01:21:35.2 -- a known variable star
06:51:28.85 -00:00:28.7 -- a known variable star
06:52:51.70 -02:22:43.9 -- not a known variable star
06:53:36.78 -02:31:44.3 -- a known variable star
06:53:46.02 -00:14:35.2 -- not a known variable star
06:53:55.08 +02:25:33.0 -- a known variable star
06:55:38.92 -06:15:20.8 -- not a known variable star
06:56:21.96 -00:53:11.0 -- a known variable star
06:56:42.67 +02:46:48.5 -- not a known variable star
06:56:45.12 +00:46:35.9 -- not a known variable star
06:57:42.55 -04:00:45.5 -- not a known variable star
06:58:09.31 -01:15:58.8 -- not a known variable star
06:58:39.23 -01:55:06.6 -- not a known variable star
06:59:09.68 +00:41:52.9 -- not a known variable star
06:59:29.48 +02:30:33.3 -- not a known variable star
06:59:34.41 +02:03:39.0 -- not a known variable star
06:59:40.23 -00:39:47.2 -- not a known variable star
07:00:09.60 -00:53:36.6 -- not a known variable star
07:00:51.57 +01:33:15.9 -- not a known variable star
07:01:00.94 -00:25:43.7 -- not a known variable star
07:01:14.48 +00:57:27.9 -- not a known variable star
07:01:21.72 +02:15:51.4 -- a known variable star
07:01:56.24 -02:41:24.4 -- not a known variable star
07:02:14.49 -03:05:56.6 -- not a known variable star
07:02:21.48 -04:03:29.9 -- a known variable star
07:02:30.67 -03:26:39.2 -- not a known variable star
07:03:07.68 -06:51:54.1 -- a known variable star
07:03:11.48 +01:23:09.8 -- a known variable star
07:03:23.99 -02:49:51.6 -- not a known variable star
07:04:11.71 -01:14:18.4 -- a known variable star
07:04:35.22 +02:44:56.4 -- a known variable star
07:04:39.04 -04:57:05.5 -- not a known variable star
07:05:00.36 -02:02:17.7 -- a known variable star
07:05:14.71 +00:02:16.2 -- not a known variable star
07:05:15.60 +00:02:29.2 -- not a known variable star
07:05:18.16 -01:22:58.4 -- a known variable star
07:05:50.95 -02:05:12.3 -- not a known variable star
07:06:06.05 -05:15:50.3 -- not a known variable star
07:06:54.61 -04:13:50.7 -- not a known variable star
07:07:24.30 +02:31:24.7 -- not a known variable star
07:07:26.04 -01:50:45.3 -- not a known variable star
07:07:58.87 -02:58:38.3 -- not a known variable star
07:08:08.39 -03:34:58.8 -- a known variable star
07:08:35.58 +01:46:44.9 -- not a known variable star
07:08:45.30 +00:41:47.8 -- a known variable star
07:09:03.33 -02:29:06.4 -- not a known variable star
07:09:13.71 -02:21:30.7 -- a known variable star
07:09:20.59 +02:38:44.5 -- not a known variable star
07:09:43.85 -01:26:40.3 -- not a known variable star
07:09:57.25 -01:59:05.8 -- not a known variable star
07:09:57.98 +00:39:41.7 -- not a known variable star
07:10:37.57 -04:15:16.6 -- not a known variable star
07:10:59.18 -03:55:09.2 -- not a known variable star
07:11:00.56 -02:53:39.2 -- not a known variable star
07:11:05.25 -04:42:12.3 -- not a known variable star
07:11:54.51 +00:45:39.1 -- a known variable star
07:13:04.72 -05:12:24.0 -- a known variable star
07:13:31.49 -03:31:14.5 -- not a known variable star
07:13:32.91 +00:13:00.8 -- not a known variable star
07:14:00.00 -02:51:46.9 -- not a known variable star
07:14:13.13 -01:59:27.9 -- a known variable star
07:16:03.90 +02:09:51.0 -- not a known variable star
07:16:33.92 -05:05:59.1 -- a known variable star
07:17:04.21 -04:46:11.1 -- not a known variable star
07:17:13.72 +02:22:35.4 -- a known variable star
07:17:30.87 +01:05:34.5 -- a known variable star
07:17:33.93 -02:54:19.7 -- a known variable star
07:17:38.05 +01:13:00.8 -- not a known variable star
07:17:39.07 -03:44:22.0 -- a known variable star
07:17:51.14 -01:41:37.5 -- a known variable star
07:17:52.75 +00:17:04.1 -- a known variable star
07:18:20.69 -04:33:00.2 -- a known variable star
07:18:41.90 +01:11:03.4 -- a known variable star
07:18:50.05 -05:15:16.6 -- not a known variable star
07:18:56.39 -04:19:24.8 -- a known variable star
07:19:20.14 -00:18:59.1 -- a known variable star
07:19:35.86 -01:56:19.0 -- not a known variable star
07:20:04.04 +02:27:50.8 -- not a known variable star
07:20:04.65 +02:28:16.8 -- not a known variable star
07:21:14.19 -02:12:39.7 -- not a known variable star
07:22:14.40 -00:18:40.7 -- not a known variable star
Found 83 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
123 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 123 (excluding asteroids and hot pixels, 83 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461144.61085134 -observatory V36
23:57:27.90 -03:03:57.0 Mercury (0.1mag)
02:59:26.01 +17:08:12.9 Venus (-3.9mag)
00:12:28.35 +00:16:26.2 Mars (1.2mag)
07:11:47.46 +22:47:36.2 Jupiter (-2.1mag)
00:28:20.25 +00:43:42.9 Saturn (0.9mag)
03:47:18.13 +19:46:12.6 Uranus (5.8mag)
00:10:35.53 -00:16:56.1 Neptune (7.8mag)
20:33:40.12 -22:52:31.4 Pluto (14.5mag)
22:42:23.52 -08:18:35.4 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 13 22:28 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461144.61085134:
07:11:42.57 +22:47:48.1 Io (5.8mag)
07:11:47.50 +22:47:33.0 Europa (5.9mag)
07:11:55.01 +22:47:27.4 Ganymede (5.3mag)
07:12:13.26 +22:46:50.7 Callisto (6.6mag)
07:15:12.60 +22:36:07.1 Himalia (15.3mag)
07:11:45.05 +22:47:39.5 Thebe (16.2mag)
07:15:21.51 +23:06:09.4 Elara (17.3mag)
07:10:32.63 +23:28:35.9 Pasiphae (17.4mag)
07:20:09.66 +22:45:26.2 Carme (18.5mag)
00:28:28.43 +00:43:58.7 Titan (8.8mag)
00:28:22.73 +00:43:56.2 Rhea (10.1mag)
00:28:03.67 +00:44:10.4 Iapetus (11.5mag)
00:28:33.66 +00:43:51.5 Hyperion (14.8mag)
00:29:58.63 +00:52:43.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 22:29 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.61085134:
15:29:52.82 -14:52:34.2 JWST
16:54:28.02 +44:52:39.1 Chandra
07:50:32.07 -33:10:55.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 22:28 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.61085134 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:12.42 -28:40:08.1 13.9mag P/2010 H2 (Vales)
05:05:23.32 -69:45:06.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:02.64 +31:25:28.9 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.57 +10:19:24.5 17.6mag C/2021 G2 (ATLAS)
23:09:42.87 +29:09:16.7 17.1mag C/2022 E2 (ATLAS)
04:27:02.33 +25:59:13.4 16.0mag C/2022 N2 (PANSTARRS)
09:03:01.76 +32:00:19.0 16.2mag C/2022 QE78 (ATLAS)
08:30:47.62 -00:21:14.8 17.3mag C/2022 R6 (PANSTARRS)
18:54:10.08 +18:22:24.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:16.72 -11:32:57.0 17.5mag P/2023 B1 (PANSTARRS)
09:08:31.61 -12:11:13.0 17.6mag C/2023 F3 (ATLAS)
21:52:17.73 +62:47:47.7 17.5mag C/2023 H5 (Lemmon)
19:20:47.92 -03:42:08.7 14.2mag C/2023 R1 (PANSTARRS)
21:35:58.83 +85:39:02.0 17.8mag C/2023 X2 (Lemmon)
06:17:02.77 +63:31:19.8 17.1mag C/2024 A1 (ATLAS)
05:09:11.67 +17:40:03.4 10.9mag C/2024 E1 (Wierzchos)
16:20:28.81 +06:04:50.4 17.4mag C/2024 G6 (ATLAS)
20:20:16.19 +14:45:46.6 14.6mag C/2024 J3 (ATLAS)
03:24:40.56 -22:40:26.8 16.4mag C/2024 T5 (ATLAS)
05:15:06.95 +45:45:45.5 17.7mag C/2025 J1 (Borisov)
13:46:41.45 +44:12:41.1 15.1mag C/2025 L1 (ATLAS)
03:22:18.13 -25:55:07.0 17.8mag C/2025 Q3 (ATLAS)
23:28:19.96 +19:09:22.9 8.8mag C/2025 R3 (PANSTARRS)
12:54:56.31 +02:53:50.5 17.4mag C/2025 Y1 (ATLAS)
03:11:37.28 +02:50:33.4 12.7mag C/2026 A1 (MAPS)
23:54:11.87 +36:52:04.1 14.5mag C/2026 B2 (Sun-Gao)
18:39:15.37 -09:49:11.4 11.9mag 10P/Tempel
15:02:51.49 +03:24:11.1 13.8mag 24P/Schaumasse
11:03:18.95 -01:35:15.0 15.7mag 29P/Schwassmann-Wachmann
18:00:23.06 -09:40:48.4 17.9mag 40P/Vaisala
10:37:39.90 -04:15:02.2 16.9mag 43P/Wolf-Harrington
01:45:44.93 +17:09:55.2 17.2mag 47P/Ashbrook-Jackson
07:07:17.45 +37:25:05.6 17.0mag 63P/Wild
23:26:38.52 -11:40:41.9 15.7mag 65P/Gunn
03:58:12.77 +20:36:09.8 15.9mag 76P/West-Kohoutek-Ikemura
01:01:23.98 +07:51:25.7 14.3mag 78P/Gehrels
22:57:15.86 -09:56:59.1 14.6mag 88P/Howell
02:05:03.74 +20:08:13.6 15.1mag 93P/Lovas
04:51:15.21 +32:11:11.4 16.2mag 123P/West-Hartley
08:26:09.78 +39:13:59.5 16.2mag 124P/Mrkos
02:30:17.85 +14:09:32.3 16.4mag 128P/Shoemaker-Holt
02:43:49.87 +14:15:43.2 17.5mag 131P/Mueller
01:16:15.61 +12:34:47.3 10.7mag 141P/Machholz
01:25:26.86 +04:09:52.3 10.7mag 141P-A/Machholz
00:11:39.75 +00:08:42.2 13.0mag 141P-D/Machholz
01:55:36.68 +05:55:01.8 17.8mag 141P-I/Machholz
00:57:06.54 -02:28:32.7 15.1mag 162P/SidingSpring
10:29:06.65 +30:57:43.9 18.0mag 164P/Christensen
06:33:02.25 +24:18:05.7 18.0mag 198P/ODAS
14:54:47.67 -00:15:56.2 17.6mag 210P/Christensen
21:33:20.72 -11:54:15.2 17.6mag 218P/LINEAR
17:16:03.58 -14:09:34.5 16.1mag 235P/LINEAR
05:30:24.44 +34:33:14.0 16.7mag 240P/NEAT
07:37:34.54 -05:22:22.4 17.7mag 242P/Spahr
22:12:11.10 -21:28:46.0 17.9mag 260P/McNaught
15:43:22.27 +06:51:54.6 17.5mag 391P/Kowalski
07:33:28.82 +21:21:35.2 17.7mag 450P/LONEOS
05:33:07.24 +45:08:36.5 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 22:28 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
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
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
-rw-r--r-- 1 apache apache 5.8K Apr 13 22:28 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 13 22:28 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
20:29:30.119 -10:56:33.33 AT 2026iuw 2026-03-29.79 19.55
13:31:30.960 -32:00:09.92 AT 2026iuv 2026-04-07.60 18.91
14:00:56.468 -25:06:29.29 AT 2026iuu 2026-04-07.35 18.482
13:27:25.132 +09:30:53.72 AT 2026iut 2026-04-05.33 19.4971
13:57:28.106 -31:36:18.49 AT 2026ius 2026-04-07.61 19.27
09:54:32.050 -01:17:25.84 SN 2026iur 2026-04-07.01 15.9
14:24:08.131 +22:56:14.71 AT 2026iuq 2026-04-07.38 19.91
10:07:28.221 -17:12:04.00 AT 2026iup 2026-04-05.31 20.26
16:21:33.361 +42:39:39.49 AT 2026iuo 2026-04-02.59 20.72
11:27:41.500 -35:48:12.21 AT 2026iun 2026-03-30.51 19.56
13:57:31.503 -10:38:39.68 AT 2026ium 2026-03-29.71 19.95
19:51:44.150 +31:28:49.50 AT 2026iul 2026-04-07.40 15.7
-rw-r--r-- 1 apache apache 30K Apr 13 22:28 tns_transients_list.txt
