This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4403+02.8930,2461149.6141,11.92,0.05,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
ATO J100.4403+02.8930 20260419.1141 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 3126272545479831808,2461149.6141,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126272545479831808 20260419.1141 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112299500737047808,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112299500737047808 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107253124624862336,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107253124624862336 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9028+01.7016,2461149.6141,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9028+01.7016 20260419.1141 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3500-01.6273,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3500-01.6273 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112515039375055744,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112515039375055744 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5006-01.4700,2461149.6141,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.5006-01.4700 20260419.1141 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5061+01.6323,2461149.6141,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.5061+01.6323 20260419.1141 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113858951823160192,2461149.6141,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113858951823160192 20260419.1141 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8479+00.5677,2461149.6141,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8479+00.5677 20260419.1141 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0656420-021737,2461149.6141,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0656420-021737 20260419.1141 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108790478098341120,2461149.6141,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108790478098341120 20260419.1141 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5364-01.5315,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.5364-01.5315 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J063732.66+014639.0,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J063732.66+014639.0 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2008-01.0734,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2008-01.0734 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107276965980840064,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107276965980840064 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0982+00.9925,2461149.6141,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0982+00.9925 20260419.1141 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109157925439214720,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109157925439214720 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109112089548511488,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109112089548511488 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3532-03.2181,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3532-03.2181 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107637197783360768,2461149.6141,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107637197783360768 20260419.1141 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9388-05.7085,2461149.6141,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9388-05.7085 20260419.1141 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113991000596997504,2461149.6141,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113991000596997504 20260419.1141 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4167-01.6943,2461149.6141,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.4167-01.6943 20260419.1141 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.8653-02.7557,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.8653-02.7557 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115631128348858368,2461149.6141,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115631128348858368 20260419.1141 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3062-02.3749,2461149.6141,13.29,0.05,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
ATO J109.3062-02.3749 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8115+03.1405,2461149.6141,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.8115+03.1405 20260419.1141 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071954.72-010006.4,2461149.6141,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071954.72-010006.4 20260419.1141 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0653348-013503,2461149.6141,13.29,0.05,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
GDS_J0653348-013503 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.1619-00.6396,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.1619-00.6396 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1424-03.8994,2461149.6141,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1424-03.8994 20260419.1141 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064630.95+010809.2,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064630.95+010809.2 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3124296963600783616,2461149.6141,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3124296963600783616 20260419.1141 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4280-01.9828,2461149.6141,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4280-01.9828 20260419.1141 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113266766033871616,2461149.6141,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113266766033871616 20260419.1141 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112536277993759872,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112536277993759872 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113790030488561920,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113790030488561920 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2029+02.1494,2461149.6141,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2029+02.1494 20260419.1141 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119827719414785920,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119827719414785920 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125562260967323136,2461149.6141,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125562260967323136 20260419.1141 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125849023043907328,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125849023043907328 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112672888012933248,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112672888012933248 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2123-01.4941,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2123-01.4941 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126155688009474560,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126155688009474560 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063753.27-055523.1,2461149.6141,13.12,0.05,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
ASASSN-V J063753.27-055523.1 20260419.1141 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113254808845036928,2461149.6141,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113254808845036928 20260419.1141 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107406673992729472,2461149.6141,13.10,0.05,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 3107406673992729472 20260419.1141 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
target,2461149.6141,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113090775451245568,2461149.6141,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113090775451245568 20260419.1141 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127222660966365824,2461149.6141,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127222660966365824 20260419.1141 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5414-00.0643,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5414-00.0643 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109451014007852160,2461149.6141,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109451014007852160 20260419.1141 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114516910751071104,2461149.6141,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114516910751071104 20260419.1141 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J071735.90-002406.8,2461149.6141,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J071735.90-002406.8 20260419.1141 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111507508770537216,2461149.6141,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111507508770537216 20260419.1141 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111108768303524224,2461149.6141,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111108768303524224 20260419.1141 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5396-00.9195,2461149.6141,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5396-00.9195 20260419.1141 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111021460208725376,2461149.6141,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111021460208725376 20260419.1141 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053137430050444416,2461149.6141,13.04,0.05,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 3053137430050444416 20260419.1141 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 3126199354937805952,2461149.6141,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126199354937805952 20260419.1141 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114074769639625216,2461149.6141,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114074769639625216 20260419.1141 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9152-04.6412,2461149.6141,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9152-04.6412 20260419.1141 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114569137555198464,2461149.6141,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114569137555198464 20260419.1141 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.1701-03.5709,2461149.6141,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.1701-03.5709 20260419.1141 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101618780365036416,2461149.6141,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101618780365036416 20260419.1141 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107947977311377408,2461149.6141,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107947977311377408 20260419.1141 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115491868329337088,2461149.6141,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115491868329337088 20260419.1141 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 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 3113323322162357504,2461149.6141,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113323322162357504 20260419.1141 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108002544877231872,2461149.6141,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108002544877231872 20260419.1141 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4191-04.3825,2461149.6141,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4191-04.3825 20260419.1141 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.8492-02.7067,2461149.6141,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.8492-02.7067 20260419.1141 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.7832-00.2755,2461149.6141,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.7832-00.2755 20260419.1141 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105564412201090816,2461149.6141,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105564412201090816 20260419.1141 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.3925-03.5224,2461149.6141,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.3925-03.5224 20260419.1141 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 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 3119584113167330944,2461149.6141,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119584113167330944 20260419.1141 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0896-02.7869,2461149.6141,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0896-02.7869 20260419.1141 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0654541-053717,2461149.6141,12.78,0.05,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
GDS_J0654541-053717 20260419.1141 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107274358943072000,2461149.6141,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107274358943072000 20260419.1141 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101503262931006720,2461149.6141,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503262931006720 20260419.1141 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.69,0.05,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 20260419.1141 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 3107638812691198208,2461149.6141,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107638812691198208 20260419.1141 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107197805444320128,2461149.6141,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107197805444320128 20260419.1141 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
target,2461149.6141,12.64,0.05,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 20260419.1141 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 J102.3654+02.4200,2461149.6141,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.3654+02.4200 20260419.1141 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
target,2461149.6141,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9286-02.2751,2461149.6141,12.59,0.05,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
ATO J107.9286-02.2751 20260419.1141 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
target,2461149.6141,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 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,2461149.6141,12.48,0.05,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 20260419.1141 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 3107928495341091456,2461149.6141,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107928495341091456 20260419.1141 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
target,2461149.6141,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115543300556247680,2461149.6141,12.48,0.05,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 3115543300556247680 20260419.1141 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 J102.8710+01.9494,2461149.6141,12.46,0.05,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 J102.8710+01.9494 20260419.1141 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 3126442553166925312,2461149.6141,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126442553166925312 20260419.1141 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461149.6141,12.37,0.05,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
ATO J098.7797-03.0546 20260419.1141 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 3113577000111038080,2461149.6141,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113577000111038080 20260419.1141 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112954191193204096,2461149.6141,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112954191193204096 20260419.1141 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9704+01.3011,2461149.6141,12.31,0.05,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
ATO J100.9704+01.3011 20260419.1141 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
ATO J107.7416-04.3083,2461149.6141,12.29,0.05,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
ATO J107.7416-04.3083 20260419.1141 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 3112130214607270656,2461149.6141,12.18,0.05,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 3112130214607270656 20260419.1141 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 J104.7305-03.0153,2461149.6141,12.17,0.05,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 J104.7305-03.0153 20260419.1141 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108867959307360128,2461149.6141,12.02,0.05,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
Gaia DR3 3108867959307360128 20260419.1141 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 3107031877968344192,2461149.6141,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107031877968344192 20260419.1141 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 3059365613665871360,2461149.6141,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059365613665871360 20260419.1141 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5177-01.4272,2461149.6141,12.08,0.05,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 J109.5177-01.4272 20260419.1141 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12675437,2461149.6141,12.02,0.05,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
NSVS 12675437 20260419.1141 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 J104.8986+00.1116,2461149.6141,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8986+00.1116 20260419.1141 11.79CV 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
GDS_J0640542+000137,2461149.6141,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0640542+000137 20260419.1141 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0653-02.3877,2461149.6141,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0653-02.3877 20260419.1141 11.76CV 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 J105.9684+00.8315,2461149.6141,11.75,0.05,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 J105.9684+00.8315 20260419.1141 11.75CV 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
NSVS 12569794,2461149.6141,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12569794 20260419.1141 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6522-00.6011,2461149.6141,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6522-00.6011 20260419.1141 11.66CV 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 3109199054047735936,2461149.6141,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109199054047735936 20260419.1141 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111060630310108928,2461149.6141,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111060630310108928 20260419.1141 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109303606430140928,2461149.6141,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109303606430140928 20260419.1141 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113665785673343744,2461149.6141,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113665785673343744 20260419.1141 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062757.74+025622.5,2461149.6141,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062757.74+025622.5 20260419.1141 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112276892032630400,2461149.6141,11.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112276892032630400 20260419.1141 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822923819222400,2461149.6141,9.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822923819222400 20260419.1141 9.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119852462723061120,2461149.6141,9.79,0.05,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 3119852462723061120 20260419.1141 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.0773+01.7811,2461149.6141,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.0773+01.7811 20260419.1141 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1631+01.7787,2461149.6141,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260419.1141 11.27CV 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 3127192493115969152,2461149.6141,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127192493115969152 20260419.1141 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
CD Mon,2461149.6141,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260419.1141 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0231-03.3091,2461149.6141,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0231-03.3091 20260419.1141 11.66CV 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 3108862088093246080,2461149.6141,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108862088093246080 20260419.1141 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115211321064418944,2461149.6141,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115211321064418944 20260419.1141 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 3111447039926977152,2461149.6141,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111447039926977152 20260419.1141 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.4987-02.8566,2461149.6141,12.04,0.05,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
ATO J108.4987-02.8566 20260419.1141 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 3112231300951646592,2461149.6141,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112231300951646592 20260419.1141 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3035-03.3194,2461149.6141,12.22,0.05,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 J106.3035-03.3194 20260419.1141 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 3059182270101246208,2461149.6141,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059182270101246208 20260419.1141 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126248970398055808,2461149.6141,12.24,0.05,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 3126248970398055808 20260419.1141 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052121068980616576,2461149.6141,12.34,0.05,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 3052121068980616576 20260419.1141 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
Gaia DR3 3108912390749031168,2461149.6141,12.32,0.05,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 3108912390749031168 20260419.1141 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 3059651314888833408,2461149.6141,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059651314888833408 20260419.1141 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 3059463538922588672,2461149.6141,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059463538922588672 20260419.1141 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.27,0.05,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
target 20260419.1141 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
ATO J110.0194-01.8183,2461149.6141,12.46,0.05,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 J110.0194-01.8183 20260419.1141 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 3053264973402395520,2461149.6141,12.46,0.05,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 3053264973402395520 20260419.1141 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 3108015429780459520,2461149.6141,12.34,0.05,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 3108015429780459520 20260419.1141 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
Gaia DR3 3108522231621317504,2461149.6141,12.46,0.05,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 3108522231621317504 20260419.1141 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 3110294236346089344,2461149.6141,12.37,0.05,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
Gaia DR3 3110294236346089344 20260419.1141 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 J105.9816-06.0164,2461149.6141,12.46,0.05,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 J105.9816-06.0164 20260419.1141 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 J109.7065-05.2541,2461149.6141,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7065-05.2541 20260419.1141 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.5120+00.7391,2461149.6141,12.38,0.05,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 J110.5120+00.7391 20260419.1141 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2174-00.5958,2461149.6141,12.46,0.05,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 J105.2174-00.5958 20260419.1141 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 3059490751835095936,2461149.6141,12.57,0.05,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 3059490751835095936 20260419.1141 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 J104.7374-04.6394,2461149.6141,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7374-04.6394 20260419.1141 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107955953073281024,2461149.6141,12.57,0.05,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 3107955953073281024 20260419.1141 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
Gaia DR3 3126445855999311744,2461149.6141,12.57,0.05,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 3126445855999311744 20260419.1141 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
Gaia DR3 3112749274012032640,2461149.6141,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112749274012032640 20260419.1141 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110006336102386176,2461149.6141,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110006336102386176 20260419.1141 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114520003127512192,2461149.6141,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114520003127512192 20260419.1141 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109532137349277568,2461149.6141,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109532137349277568 20260419.1141 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070449.39+023047.8,2461149.6141,12.61,0.05,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
ASASSN-V J070449.39+023047.8 20260419.1141 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109346732203582208,2461149.6141,12.77,0.05,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 3109346732203582208 20260419.1141 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 J106.0676-03.0161,2461149.6141,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260419.1141 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110295679455096320,2461149.6141,12.66,0.05,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 3110295679455096320 20260419.1141 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6477-03.4721,2461149.6141,12.66,0.05,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
ATO J100.6477-03.4721 20260419.1141 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1505+01.7467,2461149.6141,12.59,0.05,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
ATO J101.1505+01.7467 20260419.1141 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1999-01.8082,2461149.6141,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1999-01.8082 20260419.1141 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 J108.8701-01.1937,2461149.6141,12.64,0.05,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 J108.8701-01.1937 20260419.1141 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 3109841924755441024,2461149.6141,12.66,0.05,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 3109841924755441024 20260419.1141 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1353+02.4543,2461149.6141,12.69,0.05,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 J105.1353+02.4543 20260419.1141 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 3112760647085290752,2461149.6141,12.77,0.05,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 3112760647085290752 20260419.1141 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109297872654329344,2461149.6141,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109297872654329344 20260419.1141 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107474882374152960,2461149.6141,12.69,0.05,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
Gaia DR3 3107474882374152960 20260419.1141 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 3109190670271735936,2461149.6141,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109190670271735936 20260419.1141 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0471-05.0754,2461149.6141,12.66,0.05,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
ATO J106.0471-05.0754 20260419.1141 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 3115633327372214656,2461149.6141,12.82,0.05,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
Gaia DR3 3115633327372214656 20260419.1141 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 3113103071939549184,2461149.6141,12.79,0.05,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 3113103071939549184 20260419.1141 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
GDS_J0707331-032533,2461149.6141,12.65,0.05,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
GDS_J0707331-032533 20260419.1141 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
target,2461149.6141,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2998-03.9607,2461149.6141,12.82,0.05,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 J104.2998-03.9607 20260419.1141 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 3120812576892617856,2461149.6141,12.82,0.05,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
Gaia DR3 3120812576892617856 20260419.1141 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 3105302487915881984,2461149.6141,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105302487915881984 20260419.1141 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
ATO J107.0154-01.7229,2461149.6141,12.95,0.05,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
ATO J107.0154-01.7229 20260419.1141 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120480691881910656,2461149.6141,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120480691881910656 20260419.1141 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1615-01.5148,2461149.6141,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1615-01.5148 20260419.1141 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 3108625826231054976,2461149.6141,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108625826231054976 20260419.1141 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101029201615746048,2461149.6141,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101029201615746048 20260419.1141 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115421087268758272,2461149.6141,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115421087268758272 20260419.1141 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6876-01.5149,2461149.6141,12.85,0.05,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 J106.6876-01.5149 20260419.1141 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 3108425204019105664,2461149.6141,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108425204019105664 20260419.1141 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461149.6141,12.84,0.05,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 3126271617766100608 20260419.1141 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108090471452077184,2461149.6141,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108090471452077184 20260419.1141 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109836083598822272,2461149.6141,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109836083598822272 20260419.1141 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MGAB-V1900,2461149.6141,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MGAB-V1900 20260419.1141 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9776-05.0786,2461149.6141,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9776-05.0786 20260419.1141 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115517943069337344,2461149.6141,12.84,0.05,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 3115517943069337344 20260419.1141 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
ATO J107.2944-04.9257,2461149.6141,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2944-04.9257 20260419.1141 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107553875417557888,2461149.6141,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107553875417557888 20260419.1141 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.7055+02.5174,2461149.6141,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J097.7055+02.5174 20260419.1141 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126952627779842688,2461149.6141,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126952627779842688 20260419.1141 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106340014576032512,2461149.6141,13.04,0.05,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 3106340014576032512 20260419.1141 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 J107.6148+02.3383,2461149.6141,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6148+02.3383 20260419.1141 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108661461582071936,2461149.6141,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108661461582071936 20260419.1141 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3118345204080317440,2461149.6141,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3118345204080317440 20260419.1141 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115039350573052160,2461149.6141,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115039350573052160 20260419.1141 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126002336198034048,2461149.6141,13.04,0.05,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 3126002336198034048 20260419.1141 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 3107920768701471488,2461149.6141,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107920768701471488 20260419.1141 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112636294895145472,2461149.6141,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112636294895145472 20260419.1141 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070654.13+021046.6,2461149.6141,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070654.13+021046.6 20260419.1141 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110689064100344576,2461149.6141,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110689064100344576 20260419.1141 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109541822495218944,2461149.6141,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109541822495218944 20260419.1141 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100477590376004224,2461149.6141,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100477590376004224 20260419.1141 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113913996125565440,2461149.6141,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260419.1141 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461149.6141,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108863080225629056 20260419.1141 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 3109796982216210048,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109796982216210048 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125607134785759744,2461149.6141,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125607134785759744 20260419.1141 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125637852391270784,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125637852391270784 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114067687234902528,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114067687234902528 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9279-01.2566,2461149.6141,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9279-01.2566 20260419.1141 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.9196-05.3884,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.9196-05.3884 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3052172333716931200,2461149.6141,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3052172333716931200 20260419.1141 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3061635280540436864,2461149.6141,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3061635280540436864 20260419.1141 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 352,2461149.6141,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 352 20260419.1141 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2427-02.0482,2461149.6141,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2427-02.0482 20260419.1141 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114478256045530880,2461149.6141,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114478256045530880 20260419.1141 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127203655728648192,2461149.6141,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127203655728648192 20260419.1141 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109756094127017600,2461149.6141,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109756094127017600 20260419.1141 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108917372911018368,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108917372911018368 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113615826614868864,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113615826614868864 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106831938650976384,2461149.6141,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106831938650976384 20260419.1141 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109309692404188032,2461149.6141,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109309692404188032 20260419.1141 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108081194321500032,2461149.6141,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108081194321500032 20260419.1141 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127840174182358016,2461149.6141,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127840174182358016 20260419.1141 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.2733+03.1310,2461149.6141,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.2733+03.1310 20260419.1141 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108460491469971584,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108460491469971584 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127836875647223296,2461149.6141,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127836875647223296 20260419.1141 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112852799904385536,2461149.6141,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112852799904385536 20260419.1141 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125762818759967104,2461149.6141,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125762818759967104 20260419.1141 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107712170734171776,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107712170734171776 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106199856901798528,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106199856901798528 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059434126986016128,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059434126986016128 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114460526421262848,2461149.6141,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114460526421262848 20260419.1141 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102263231617910528,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102263231617910528 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113525082544566656,2461149.6141,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113525082544566656 20260419.1141 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112456559100452352,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112456559100452352 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.1511-05.8493,2461149.6141,13.29,0.05,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
ATO J109.1511-05.8493 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7479+00.9409,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7479+00.9409 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.1862-05.0049,2461149.6141,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.1862-05.0049 20260419.1141 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106229822896913792,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106229822896913792 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111161574920855808,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111161574920855808 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102125311628346112,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102125311628346112 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3061678539451225600,2461149.6141,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3061678539451225600 20260419.1141 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106045203719510272,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106045203719510272 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107172379238302208,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107172379238302208 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111159380198287232,2461149.6141,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111159380198287232 20260419.1141 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100441267835993600,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100441267835993600 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109084876636349440,2461149.6141,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109084876636349440 20260419.1141 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113219246514568576,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063845.97+020335.5,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063845.97+020335.5 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108952965300016384,2461149.6141,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108952965300016384 20260419.1141 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109301102469733120,2461149.6141,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109301102469733120 20260419.1141 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125817485103519104,2461149.6141,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125817485103519104 20260419.1141 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.5776-03.3486,2461149.6141,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.5776-03.3486 20260419.1141 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7533-02.6015,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7533-02.6015 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.7297-02.0389,2461149.6141,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.7297-02.0389 20260419.1141 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113408362514158720,2461149.6141,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113408362514158720 20260419.1141 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104963529097936256,2461149.6141,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3104963529097936256 20260419.1141 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119355071151771648,2461149.6141,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119355071151771648 20260419.1141 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114315665764303488,2461149.6141,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114315665764303488 20260419.1141 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
[KEE2007] 2083,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
[KEE2007] 2083 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113342490594252544,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113342490594252544 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126954478907174144,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126954478907174144 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TY Mon,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TY Mon 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063257.40-022316.5,2461149.6141,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063257.40-022316.5 20260419.1141 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108108819552214400,2461149.6141,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108108819552214400 20260419.1141 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115536462968304768,2461149.6141,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115536462968304768 20260419.1141 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9025+01.8704,2461149.6141,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9025+01.8704 20260419.1141 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.7790+02.9110,2461149.6141,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.7790+02.9110 20260419.1141 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.8569-05.9675,2461149.6141,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.8569-05.9675 20260419.1141 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113470691079092224,2461149.6141,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113470691079092224 20260419.1141 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4997-02.1281,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4997-02.1281 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114787734210014720,2461149.6141,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114787734210014720 20260419.1141 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.5625+00.7298,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.5625+00.7298 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113651900038506752,2461149.6141,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113651900038506752 20260419.1141 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113313186039752960,2461149.6141,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113313186039752960 20260419.1141 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0652-01.8288,2461149.6141,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0652-01.8288 20260419.1141 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2019-03.5474,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2019-03.5474 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461149.6141,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260419.1141 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9614-02.2114,2461149.6141,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9614-02.2114 20260419.1141 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J065633+0239.5,2461149.6141,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J065633+0239.5 20260419.1141 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.8637-03.6635,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.8637-03.6635 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100960241622195968,2461149.6141,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100960241622195968 20260419.1141 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106850291050328576,2461149.6141,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106850291050328576 20260419.1141 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107426121606726016,2461149.6141,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107426121606726016 20260419.1141 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.2855+02.6985,2461149.6141,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.2855+02.6985 20260419.1141 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115653805774968832,2461149.6141,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115653805774968832 20260419.1141 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7908-02.3649,2461149.6141,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7908-02.3649 20260419.1141 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8633+01.2636,2461149.6141,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8633+01.2636 20260419.1141 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.1141* 06 20 28.15 -03 16 34.6 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461149.6141,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.9442+01.1817,2461149.6141,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.9442+01.1817 20260419.1141 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3533-02.2202,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3533-02.2202 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065811.83-022600.0,2461149.6141,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065811.83-022600.0 20260419.1141 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106352487161144960,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106352487161144960 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112342935747518720,2461149.6141,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112342935747518720 20260419.1141 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102623076859922432,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102623076859922432 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J070938.64-000118.1,2461149.6141,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J070938.64-000118.1 20260419.1141 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112632309164197888,2461149.6141,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112632309164197888 20260419.1141 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0837+00.8377,2461149.6141,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0837+00.8377 20260419.1141 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.1082-03.9124,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.1082-03.9124 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4327-02.3509,2461149.6141,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4327-02.3509 20260419.1141 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.0517+00.0791,2461149.6141,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.0517+00.0791 20260419.1141 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9633-01.1764,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9633-01.1764 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114022748995757568,2461149.6141,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114022748995757568 20260419.1141 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102445578751032320,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102445578751032320 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4222-03.0725,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4222-03.0725 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107455911497806848,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107455911497806848 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9357-02.5893,2461149.6141,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9357-02.5893 20260419.1141 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126366583782393984,2461149.6141,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126366583782393984 20260419.1141 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100997006542102272,2461149.6141,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100997006542102272 20260419.1141 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8375+00.5577,2461149.6141,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8375+00.5577 20260419.1141 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9434+02.6679,2461149.6141,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9434+02.6679 20260419.1141 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108042505253229952,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108042505253229952 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059574967551510784,2461149.6141,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059574967551510784 20260419.1141 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7933-01.3847,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7933-01.3847 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3113-05.3430,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3113-05.3430 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106151345251783936,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106151345251783936 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.4874+01.2254,2461149.6141,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.4874+01.2254 20260419.1141 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5413+01.6888,2461149.6141,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.5413+01.6888 20260419.1141 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.2605+02.6192,2461149.6141,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.2605+02.6192 20260419.1141 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF18acnnxav,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF18acnnxav 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127770183395674880,2461149.6141,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127770183395674880 20260419.1141 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FASTT 188,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 188 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114806906944139904,2461149.6141,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114806906944139904 20260419.1141 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2972-03.8675,2461149.6141,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2972-03.8675 20260419.1141 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112044006023794304,2461149.6141,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112044006023794304 20260419.1141 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109479773108571648,2461149.6141,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109479773108571648 20260419.1141 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7719+00.5391,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.7719+00.5391 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109432425389948800,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109432425389948800 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115602261869859584,2461149.6141,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115602261869859584 20260419.1141 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6668+00.7072,2461149.6141,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6668+00.7072 20260419.1141 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.5740+02.9880,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.5740+02.9880 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119613967480138368,2461149.6141,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119613967480138368 20260419.1141 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0680+00.8355,2461149.6141,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0680+00.8355 20260419.1141 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059623311702270848,2461149.6141,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059623311702270848 20260419.1141 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3488-02.6186,2461149.6141,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3488-02.6186 20260419.1141 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.87,0.05,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
target 20260419.1141 13.87CV 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 3113104347548016384,2461149.6141,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113104347548016384 20260419.1141 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113259619208074880,2461149.6141,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113259619208074880 20260419.1141 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106954744655946624,2461149.6141,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106954744655946624 20260419.1141 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.3737-01.0057,2461149.6141,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.3737-01.0057 20260419.1141 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1044+00.4416,2461149.6141,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1044+00.4416 20260419.1141 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106319433092617216,2461149.6141,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106319433092617216 20260419.1141 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.89,0.05,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
target 20260419.1141 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109856184046620800,2461149.6141,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109856184046620800 20260419.1141 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070254.68-013527.4,2461149.6141,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070254.68-013527.4 20260419.1141 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2145+00.8666,2461149.6141,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2145+00.8666 20260419.1141 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.1185-02.6809,2461149.6141,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1185-02.6809 20260419.1141 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.87,0.05,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
target 20260419.1141 13.87CV 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
target,2461149.6141,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6141,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1141 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126475680252025088,2461149.6141,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126475680252025088 20260419.1141 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125987733307322880,2461149.6141,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125987733307322880 20260419.1141 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461149.6141,10.32,0.05,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
AG Mon 20260419.1141 10.32CV 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
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,2461149.6141,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BM Mon 20260419.1141 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461149.6141,10.60,0.05,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
RR Mon 20260419.1141 10.60CV 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
## 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: 2461149.61452425 19.04.2026 02:44:44.895 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
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: 8 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): 35384
Objects passed selection criteria: 35333
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 32148.8
Average stars matched: 31182 (96.9929 %)
Memory usage VmPeak: 136948 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 21:47:34 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: 2461149.61452425 19.04.2026 02:44:44.895 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 985
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: 255 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): 253654
Objects passed selection criteria: 253055
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 235970
Average stars matched: 226334 (95.9165 %)
Memory usage VmPeak: 2006948 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 21:54:47 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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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: 2461149.61372226
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:27.135 -01:59:26.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.135 -01:59:26.97
Angular distance between the image centers 0.0678 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:26.313 -02:00:08.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:26.313 -02:00:08.79
Angular distance between the image centers 0.0699 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 06:51:27.135 -01:59:26.97
Second-epoch second image center 06:51:26.313 -02:00:08.79
Angular distance between the image centers 0.01211 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.J8AlcQ4pd8
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.f4QoJCRcE5
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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits &> /tmp/tmp.UlnfVSKIeE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits &> /tmp/tmp.FuzNKhCPA6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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 21 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.7 mag. fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
14.7 mag. fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.J8AlcQ4pd8 (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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.f4QoJCRcE5 (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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.UlnfVSKIeE (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3235, passed=28333
Got 28333 stars (including 25079 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat
util/solve_plate_with_UCAC5 got 28333 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 26450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 930 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(), 26450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 26449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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.FuzNKhCPA6 (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3225, passed=28057
Got 28057 stars (including 24797 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat
util/solve_plate_with_UCAC5 got 28057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 26233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 26232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 26232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53466.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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 52514_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52514_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:54.25 -05:36:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.690 3101221749287884544 103.72582974552 -05.61422505292 12.3187 11.8966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:31:39.66 -05:14:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52521_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52521_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:56.01 -03:45:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.06, MAG_FAINT_SEARCH_LIMIT=12.04)GAIADR2_OUTPUT=# 1.511 3102730592781122176 103.23306216824 -03.75253037047 11.1851 10.8050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:51.33 +00:22:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.081 3113516389531142912 102.21376924338 +00.37265378636 11.0074 10.5246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52524_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52524_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:04:59.48 -05:12:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52677_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52677_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:06.42 +01:45:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52914_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52914_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:13.73 -02:21:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.14, MAG_FAINT_SEARCH_LIMIT=12.12)GAIADR2_OUTPUT=# 1.145 3108413487348260096 107.30715778798 -02.35884166817 12.0218 10.2260 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52922_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 52922_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:31.29 +01:05:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 4.596 3111748198735945984 109.38142228257 +01.09484165755 10.3371 8.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53403_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53403_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:44:47.51 -05:17:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.415 3100694670902364416 101.19783487843 -05.29681766536 10.3253 8.7996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53425_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53425_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:45.37 +00:41:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 3.050 3114302329885570688 107.18869775869 +00.69614230443 11.9358 11.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 53466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53480_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53480_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:22.02 -04:14:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.895 3059582526693134592 107.84150580449 -04.23545065630 12.1624 11.3144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:27.38 -00:31:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.377 3112612517952636288 105.86445634287 -00.52483421046 12.0598 11.6040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53484_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53484_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:48.31 -04:51:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.110 3102075039031005056 103.20101982134 -04.85629740185 12.0596 11.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:21.52 -04:23:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.580 3059485151197855232 107.58930525268 -04.38850839606 12.1625 11.8492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53545_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53545_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:57:00.66 -06:11:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.122 3100850977654068096 104.25276633181 -06.18728380277 12.3392 12.1415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53546_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53546_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:09.44 -03:05:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53552_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53552_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:32:41.38 +00:00:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53553_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53553_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:59.60 -05:32:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53560_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 53560_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:58.48 +01:25:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.189 3111669995970673664 109.99294802147 +01.42481530779 12.2878 11.6076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:53.13 -06:53:23.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 15s
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 ####
06:41:43.15 +02:53:01.3
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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:27.135 -01:59:26.97 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:27.135 -01:59:26.97
Angular distance between the image centers 0.0678 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Image size: 941.5'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:51:26.313 -02:00:08.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:26.313 -02:00:08.79
Angular distance between the image centers 0.0699 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 06:51:27.135 -01:59:26.97
Second-epoch second image center 06:51:26.313 -02:00:08.79
Angular distance between the image centers 0.01211 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.DETy1vNlBz
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.fwS3aXf6sv
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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits &> /tmp/tmp.sqkzDC6rR8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits &> /tmp/tmp.CJVfnDPMUr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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 932 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.0 mag. fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
14.0 mag. fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DETy1vNlBz (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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.fwS3aXf6sv (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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.sqkzDC6rR8 (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=71, blended=32754, passed=217186
Got 217186 stars (including 184204 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat
util/solve_plate_with_UCAC5 got 217186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 211484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 211486 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 211481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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.CJVfnDPMUr (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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=79, blended=33209, passed=218894
Got 218894 stars (including 185386 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat
util/solve_plate_with_UCAC5 got 218894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 938 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(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 212197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 212197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 212194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 938 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_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/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_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-43-35_20.00sec_-4.90C_LIGHTs_0266.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.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_2026-04-18_CI_Mon-02-Q1b1x1_214536_TTUQ1b1x1_2876113_NnxpbHdw/wcs_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288565.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out288777.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out289011.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out294988.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296267.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296398.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296701.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out296893.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out121122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296861.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296970.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 965s
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: 324s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288358_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288358_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:46.07 +02:10:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288361_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288361_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288370_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288370_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288372_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288372_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288376_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288376_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:18.60 +02:08:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288377_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:57.44 +02:26:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288378_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288378_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:37.55 +00:58:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.009 3111590801071481472 110.15602441583 +00.98028564100 14.2742 13.7324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288381_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288381_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288385_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288385_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288386_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288386_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:39:04.93 -01:14:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288388_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288388_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288389_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288389_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:17.86 +01:00:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.443 3114538041992236928 106.32396234524 +01.01196346200 14.2942 13.6836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288393_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288393_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:56:53.51 -01:17:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288398_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288398_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:39.70 -00:24:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.705 3110976895628214784 108.41493511489 -00.40129835374 14.4421 13.9643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288401_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288401_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288405_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288405_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288409_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288409_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:17.69 -02:37:06.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288411_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288411_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:13.22 +01:14:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.236 3114582434773925504 106.55495365009 +01.24055925129 14.4893 14.1499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288419_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288419_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288420_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288420_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:49.47 -00:12:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.984 3111179137047754112 107.95595298251 -00.20709329837 14.4652 14.0130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288421_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288421_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:39:49.02 +01:09:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.444 3125872112787850752 099.95380648619 +01.15118133169 14.1561 13.3983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288422_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288427_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288427_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:23:40.71 +01:04:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.483 3123462880951028608 095.91891162464 +01.06631833743 13.9175 12.9182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288431_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288431_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:11.46 -02:17:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.380 3108380330201214976 108.04737788160 -02.29574192692 14.4060 13.8861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288434_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288434_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288439_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288439_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:57:22.96 +02:20:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.030 3115736818902313856 104.34504149147 +02.33868199422 14.4822 13.9138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288440_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288440_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:25.82 -01:55:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.950 3108499214896060544 108.35694182092 -01.92202188361 14.5203 14.0340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288442_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288442_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:37.80 -00:44:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.684 3112589329430860032 105.90782726838 -00.74461208084 14.6240 14.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:15.43 +00:55:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.310 3119846071812024192 100.06409488846 +00.92053804470 14.5900 13.9776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288451_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288451_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288454_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288454_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288456_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288456_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:06.26 +01:36:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.445 3126133457258796672 102.27573289503 +01.60933180268 14.4170 13.5158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288461_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288461_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:46.58 +00:50:40.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288465_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288465_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:19.43 +01:43:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.271 3111928041903790976 109.58079360704 +01.73246549196 14.2458 13.6911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288476_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288476_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:27.15 +01:35:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 5.407 3114511172674795264 107.36255922503 +01.58449736467 14.4418 13.7019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288479_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288480_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288480_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:28.43 +03:01:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.781 3127842063967195392 103.61773770839 +03.02715183520 14.0948 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288485_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288485_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288489_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288489_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288490_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288490_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:59.39 -06:49:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.570 3099497375760475136 102.99662459991 -06.82140693975 14.2339 13.4583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288497_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288501_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288501_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:21.33 -05:32:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 4.244 3053340599185309696 107.08793569238 -05.54002383359 14.3662 14.1143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288503_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288503_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288516_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288516_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:45.76 +02:44:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.783 3127257982777240192 100.94014729133 +02.74364631956 14.0054 13.0136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288526_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288526_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288532_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288532_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288535_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288535_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288536_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288545_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288545_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:28.12 -02:23:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.699 3108835150058695552 105.86629939287 -02.39408713792 14.4402 13.9487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288547_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288547_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288548_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288548_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:11.79 +00:14:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.477 3125505739198071040 101.29884931989 +00.24208721242 14.2269 13.7415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288554_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288554_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:56.68 +02:21:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.268 3126377377041323392 101.98565435972 +02.35870851763 14.3962 13.7590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288557_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288557_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:56.60 -03:01:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.797 3107949596521735040 107.23496019636 -03.02586875566 14.3482 13.6068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288561_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288561_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288565_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288565_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:30.39 +02:24:35.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:02.78 -04:50:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.974 3059440998933764224 107.01117331229 -04.84254210889 14.4141 13.9439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:58.81 +00:32:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.680 3113765669433882496 103.49456538185 +00.53382918990 14.0458 13.1874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288575_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288575_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288576_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288576_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:01.12 +01:14:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288583_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288583_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:38.30 +01:09:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.559 3111599975121926016 110.40923219897 +01.15499300278 14.1265 13.6239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288586_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288586_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:48.91 +00:40:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.849 3111345953576489472 108.70308397131 +00.66833997778 14.2786 13.5337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288591_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288591_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288592_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288592_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:34.64 +02:03:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.629 3115660261105980160 104.89373599114 +02.06004871715 14.0627 13.5159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288597_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288597_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:49.92 -00:33:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.317 3110263548802088448 109.70750767472 -00.55550354143 14.1755 13.6634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288599_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288599_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:06.82 -02:03:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.669 3108317520603828992 108.77784480163 -02.05644199754 14.4678 14.0136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288602_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288602_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:41:02.39 +01:08:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.191 3125863454135067008 100.25961682602 +01.14441492507 14.1205 13.5264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288603_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288603_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:56:30.31 -01:05:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.415 3112410555712182144 104.12551218773 -01.09847473707 14.4552 13.5802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288604_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288606_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288609_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288609_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:18.69 +01:04:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288611_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288611_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:56.14 +01:25:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288614_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288614_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288619_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288619_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288620_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288620_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288624_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288624_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288628_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288628_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288636_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288636_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288637_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288637_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288638_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288638_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:44.16 +01:50:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.210 3135913269588830080 110.43406156313 +01.84283259987 14.3637 13.8391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288640_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288640_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:20.60 -00:26:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.153 3109705722746692864 106.83544691507 -00.43508684188 14.1682 13.2878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288641_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288641_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288645_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288645_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:48.85 +00:23:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.275 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288646_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288646_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:28.14 -01:23:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.039 3109491558499060480 106.61619134121 -01.38638838233 14.3595 13.3433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288654_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288654_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288655_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288655_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288658_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288658_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288666_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288666_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:51.30 -05:11:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288670_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288670_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:12.28 +02:10:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288672_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:48.77 -02:23:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288673_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288673_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:22:12.01 +02:04:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288676_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288676_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288679_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288679_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288680_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288680_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:03.08 +00:13:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.434 3111293211378940800 108.51222601837 +00.22645286588 14.0629 13.4039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288684_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288684_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288688_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288688_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:20.78 -00:17:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.107 3107460343905382912 101.58623755812 -00.28548509265 14.2042 13.5171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288693_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288693_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:33.78 -00:20:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288698_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288698_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:50.96 -01:23:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288699_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288699_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288707_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288707_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288708_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288708_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288710_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288710_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:19.13 +01:07:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288717_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288717_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288720_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288720_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288721_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288721_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:12.25 +00:34:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.628 3111339047269225856 108.54994317077 +00.56816531424 14.2430 13.7189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288730_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288730_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:24.75 +01:37:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.175 3125949392140417152 101.35425108516 +01.62616815977 14.1145 13.6122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288733_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288733_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:51.16 +00:10:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.051 3112979175022070272 105.46227533068 +00.16902751912 14.2083 13.6327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288734_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:54.06 +01:18:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.631 3111805240199035392 108.72485727634 +01.31366121221 14.1725 13.6944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288736_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288736_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:10.10 +02:05:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.936 3135936153174376576 110.04179012501 +02.08869676367 14.0432 13.6498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288746_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288746_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:21.57 -00:32:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288748_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288748_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:04.84 +01:22:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 4.678 3114494370763124352 107.77010562724 +01.36859081160 14.2598 13.9764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:31:44.56 +02:37:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.579 3124065310244678144 097.93525832045 +02.62637870936 13.9133 13.1167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288754_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288754_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:40.31 +01:18:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.414 3114487735035278976 107.66741265705 +01.30323744281 13.8264 13.3666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288755_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288755_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:44:44.89 +02:30:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.415 3127191629821693568 101.18715707165 +02.51383377657 14.1690 13.2618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:34.68 -01:29:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288763_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288763_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:31.56 -00:43:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.365 3110903331429336064 108.63076643940 -00.71810289053 13.9098 13.4475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288765_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288765_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:01.75 +00:37:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.923 3114297386383809152 107.00691226902 +00.62360276551 14.1345 13.6096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:37:56.07 +00:48:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288767_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288767_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288772_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288772_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:11.70 -00:03:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.449 3111177453420713856 107.54880382037 -00.05551196645 13.9330 13.1526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288773_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288773_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288775_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288775_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288777_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288777_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:01.91 -03:10:13.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288785_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288785_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:52.08 -00:10:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.787 3112849054693226496 104.96656531377 -00.17787450915 13.9712 13.1747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288787_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288788_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288788_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:29.63 +02:30:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.511 3115754509872056192 104.87304614867 +02.50886577454 13.8045 13.2690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288789_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288789_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288790_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288790_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:17.39 -04:22:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.934 3102314118390911104 103.07205510738 -04.37743286407 14.1845 13.6979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288791_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288791_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288792_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288792_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:01.08 -02:06:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288798_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288798_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288805_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288805_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:10.26 -00:32:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:04:28.43 -04:43:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.278 3101538756541332352 106.11831368719 -04.71842678074 14.0383 13.6930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288807_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288807_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288809_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288809_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:58.92 +00:11:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.829 3112759547573659008 106.49478838253 +00.18855727320 14.1112 13.5262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288814_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:04.53 +02:16:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.335 3115547874703471744 106.51825178579 +02.27236972343 14.0049 13.2415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288815_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288815_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:47.52 -05:24:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:43.13 +03:04:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288824_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288824_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288825_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288825_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:32.95 -01:17:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.142 3110070176493980416 109.13666627621 -01.29988658696 14.2421 13.8911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288835_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288837_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288837_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:05.89 -00:56:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.240 3110870002483448064 108.27457268492 -00.93492738457 14.1042 13.6373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288840_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288840_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:57.45 -02:21:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288843_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288843_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:32.63 -00:35:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.922 3110909344383313664 108.88581444280 -00.58615989687 13.8904 13.2263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288847_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288847_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288851_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288851_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288855_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288855_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288856_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288856_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288859_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288859_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:00.62 -02:27:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.562 3108382597944365184 107.75203705934 -02.45583826967 13.9392 13.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288861_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288861_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288865_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288865_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:46.29 -00:10:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.240 3110655215457441408 109.94278109384 -00.17072849306 13.8435 13.3336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288866_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288866_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:00:06.95 +02:57:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.154 3115877826971729792 105.02857894626 +02.96449349911 13.9092 13.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:51.76 +00:44:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.959 3123392817146526720 096.21537110848 +00.74862680769 13.9489 13.2916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288871_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288871_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:41.66 -04:31:44.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288874_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288874_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:41.43 -00:09:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.569 3111043205623825792 109.17189007575 -00.15297107023 13.9845 13.6973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288875_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288875_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288876_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288876_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288878_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288878_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:02:33.68 -01:57:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.250 3109049314307207680 105.63950162813 -01.96758727063 13.9169 13.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288881_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288881_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:12.58 -01:58:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288884_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288884_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288887_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288887_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288888_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288888_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:56.29 -02:14:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.679 3108251893502200192 109.48443486195 -02.24351641744 13.9286 13.2644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288890_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288890_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288891_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288891_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:15.99 +02:48:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.544 3126338722334559232 103.31631362468 +02.81242703418 13.7625 13.2418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288892_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288892_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:53.38 +01:01:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.108 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288894_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288894_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:19.88 -05:48:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288895_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288895_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:56.31 -01:57:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.230 3061734958140664448 110.23428666272 -01.96470871988 13.8898 13.4749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288896_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288896_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:42:57.07 +00:43:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.568 3125594799639377024 100.73738555000 +00.73187374331 13.4606 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288899_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288899_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:57.27 -03:17:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.078 3060069713422807296 109.73872149105 -03.29004521166 13.9133 13.2895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288900_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288900_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:24.25 +01:44:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.161 3115407858769508864 105.85054732941 +01.73724252246 13.7366 12.8891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288905_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288905_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288910_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288910_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:18.49 -02:35:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288911_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288911_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288916_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288916_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:27.63 -01:00:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.976 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288918_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288918_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288921_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288921_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288929_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288929_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:18.81 +02:45:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288933_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288933_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288937_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288937_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288939_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288939_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:39.67 -02:35:34.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288940_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288940_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:16.95 -05:34:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288943_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288943_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288944_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288944_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:57.66 +02:49:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.186 3116003347394333696 106.49042808236 +02.82051758828 13.9886 13.5116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288946_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288946_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:20.39 -02:13:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288947_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288947_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288948_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288948_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288949_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288949_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:37.05 +01:52:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288951_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288951_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:03.64 +01:06:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288952_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288952_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:22:41.85 +02:15:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288953_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288953_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288955_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288955_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288957_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288957_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288964_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288964_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288967_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288967_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288968_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288968_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288972_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288972_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:12.74 -02:21:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 4.020 3108235229029131136 109.55310949493 -02.36675533777 13.8261 13.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288973_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288973_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288975_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288975_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288980_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288980_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:59.81 +01:25:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.000 3114505228441453568 107.49856296580 +01.42885351832 13.7133 13.1674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288981_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288981_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288982_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288982_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288983_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288983_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:53.00 -01:58:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288986_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 288986_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288989_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288989_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:08.10 +02:31:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:07.68 +01:27:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288998_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288998_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:20:38.71 -06:06:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288999_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 288999_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:20.26 +01:36:10.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289000_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289000_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:52.05 -01:20:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289001_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289001_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:35:38.66 +02:05:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.813 3126928369804500736 098.91064171596 +02.09223159509 13.3570 12.3694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:59.53 -04:42:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289007_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289007_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:21.84 -03:32:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.408 3060012332660082688 108.59083691020 -03.53600984912 13.6506 12.9270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289008_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289008_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:35.65 -01:07:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 5.072 3110100546202501504 108.89714551473 -01.12785743168 13.8270 13.4399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289011_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289011_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:14.45 -00:48:25.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289013_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289013_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:57:00.81 +02:39:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.154 3127760627087443968 104.25291647070 +02.65867139961 13.8772 13.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289016_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289016_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289020_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289020_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289021_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289021_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:42:02.31 +03:04:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.916 3127470016721948672 100.50926061391 +03.07716935730 13.5539 13.1235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289024_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289024_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:45.65 -05:25:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289025_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289025_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:24.52 +00:13:20.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289026_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289026_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:33.44 -02:20:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289027_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289027_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:32.62 -01:58:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289028_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289028_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289029_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289029_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289032_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289032_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:07.73 -03:19:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:49.52 +02:13:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.534 3115664010613672832 104.95592961789 +02.21918834243 13.2142 12.3137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:59.82 -06:50:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289045_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289045_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:08.09 -03:40:03.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289046_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289046_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:22.61 +00:57:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.275 3113981792187414656 103.09343035440 +00.95023047930 13.5548 12.9216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289053_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289053_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:32.35 -04:43:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289055_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289055_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:03.74 -00:36:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.286 3109644386314358144 107.26497435016 -00.60570780031 13.6141 13.0161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289056_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289056_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289060_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289060_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:11.70 -00:21:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289061_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289061_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:59.04 -00:15:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.409 3110993727603082624 108.24539649972 -00.26542689484 13.5877 12.8049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289062_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289062_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289063_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289063_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289064_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289064_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:49.11 -05:30:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289066_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289066_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:04:35.25 +02:44:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.110 3115638962369103616 106.14639238151 +02.74839410305 13.5299 12.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289067_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289067_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:57.02 -00:27:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.812 3109703175827088256 106.98694827441 -00.46701389080 13.7069 12.9481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289072_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289072_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:46.91 +02:34:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289073_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289073_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:46.45 -01:02:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289074_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289074_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:25.59 +02:12:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289075_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289075_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:02:54.71 +01:24:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.048 3115374559882270464 105.72754735835 +01.41350873453 13.3857 12.8537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289077_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289077_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289079_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289079_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:22:43.70 -00:18:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289080_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289080_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:42.08 -01:47:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289081_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289081_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:09.66 +03:04:15.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289082_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289082_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:14.13 -02:58:54.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289084_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289084_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289085_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289085_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:59.58 +00:47:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.991 3113075652868323456 104.99767126892 +00.78455431311 13.5540 12.9503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289087_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289087_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:38.61 +02:19:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:26.96 +01:29:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.132 3114684242678561536 106.61261082895 +01.49298084908 13.4768 12.7755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289099_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289099_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289103_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289103_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289104_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289104_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289105_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289105_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:34:59.04 +02:18:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.179 3126983787762998784 098.74596416222 +02.31292312162 13.4504 12.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289106_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289106_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:09.87 -02:44:23.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289108_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289108_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289111_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289111_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289117_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289117_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:18.14 -01:22:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.841 3109471389332243584 106.32502937343 -01.38385639339 13.4701 12.9514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289120_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289120_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:32.93 +01:35:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289123_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289123_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:49.70 +03:05:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.387 3126584768121505920 102.20671844528 +03.09422588751 13.5207 13.1117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289125_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289125_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289126_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289126_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:10.16 -06:22:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.479 3052286511129009280 108.29163762548 -06.37095109742 13.4249 12.5717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289128_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289128_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:52.40 -00:04:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.473 3110297156923792640 109.71831495544 -00.07574220333 13.4389 12.7124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289129_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289129_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:56:43.65 +02:46:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.226 3127766919219874688 104.18143344956 +02.78191443907 13.3299 12.8376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289130_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289130_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289132_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289132_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:57.19 +00:37:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.707 3111516274799177600 109.23810483921 +00.62290405066 13.4683 12.7778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289136_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289136_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289138_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289138_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:10.92 -00:43:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289142_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289142_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:32.88 +00:13:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.520 3111293894273571072 108.38659943267 +00.22030237461 13.3278 13.0797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:43.67 -02:48:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289145_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289145_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:09.33 +00:52:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289152_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289152_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:17.54 -01:16:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289154_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289154_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289155_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289155_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289156_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289156_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:41:45.19 -01:18:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289157_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289157_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:56.05 -05:49:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289158_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289158_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:33.17 +00:32:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.944 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289159_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289159_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:23.29 -00:49:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 4.047 3109432047432592384 107.84649073771 -00.82722994805 13.1589 12.4319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289160_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289160_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:33.45 -02:33:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289162_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289162_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289163_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289163_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:27.06 -05:01:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289164_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289164_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:54.64 +01:48:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289165_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289165_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:42:09.78 -03:38:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.877 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289166_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289166_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:04.58 +00:48:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289168_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289168_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:57.38 -01:59:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.966 3108464614638568192 107.48875942657 -01.98545206208 13.0794 12.6389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289171_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289171_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:10.22 +00:34:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 3.572 3113585005929928448 103.04228878916 +00.57671914046 13.0745 12.6951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289174_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289174_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:17.32 -01:27:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289177_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289177_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289178_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289178_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:33.29 -02:10:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289181_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289181_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:00.03 +01:17:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289182_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289182_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289183_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289183_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:08.23 -05:53:00.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289188_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289188_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:13.46 +01:52:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289189_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289189_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289192_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289192_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289195_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289195_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289197_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289197_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289199_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289199_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:03.29 -01:37:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.395 3108536426492445952 108.51346187080 -01.62281240647 12.9032 12.2304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289201_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289201_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:56:13.95 -05:00:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289204_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289204_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:15.24 -02:52:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289205_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289205_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:52.66 -02:18:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 3.904 3108286390680405632 108.71885247002 -02.30423183879 12.2834 11.6134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289207_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289207_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:54.61 +00:53:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.758 3113971690424905728 103.47724737496 +00.88351500760 12.1834 11.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289208_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289208_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:13.90 -03:36:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 4.113 3102603805347108864 105.30706796189 -03.61185024820 12.7881 12.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289209_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289209_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:33.69 -04:55:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289210_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289210_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:02.39 -01:55:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.238 3109811997422651392 109.25974482713 -01.92788937551 12.8310 12.5097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289217_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289217_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289218_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289218_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289219_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289219_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289220_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289220_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:50.77 +01:53:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289223_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289223_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289226_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289226_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289228_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289228_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289231_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289231_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:44.74 +02:19:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289232_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289232_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289233_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289233_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:05.10 -02:00:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.928 3109208739192432768 107.27081890339 -02.00546754613 11.8572 10.7860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289236_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289236_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289237_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289237_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:25:38.43 +01:09:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 2.398 3123444670289907840 096.40986661190 +01.16585815077 12.2700 11.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289238_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289238_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:38:47.97 +00:39:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 3.295 3119814529571933824 099.69953942625 +00.66545390352 11.2963 9.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289239_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289239_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289240_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289240_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289241_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289241_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:17.79 +01:47:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289246_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289246_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:58:26.70 -00:54:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 3.076 3112253325548814208 104.61066330762 -00.91453798124 11.7888 10.7799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:51.00 -00:49:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289248_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289248_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:03.56 -04:55:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289251_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289251_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:24.38 +01:15:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289252_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289252_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:52.29 -01:57:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289253_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289253_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:59.07 -04:51:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289254_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289254_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:02.28 -02:48:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289257_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289257_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:52.50 +00:16:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 0.872 3111435834352490752 109.96898542965 +00.27883173656 11.4762 10.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289259_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289259_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 289481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289668_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289668_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:37.55 +00:27:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.24, MAG_FAINT_SEARCH_LIMIT=11.22)GAIADR2_OUTPUT=# 1.746 3114280412673080576 107.15620925738 +00.46477827338 10.8261 9.9927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289935_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289935_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:38.90 -03:56:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289962_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 289962_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:49.50 -05:43:06.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290064_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290064_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:37.29 +00:26:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.91, MAG_FAINT_SEARCH_LIMIT=11.89)GAIADR2_OUTPUT=# 2.448 3113576308614129408 102.90501560737 +00.44942258340 11.7443 11.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290168_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290168_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:39.77 +00:25:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.822 3113575518340150144 102.91541977930 +00.42535450446 11.9815 11.7792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290257_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290257_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:37.76 +00:43:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.458 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290268_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290268_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:14.55 -00:47:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290370_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290370_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290390_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290390_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290391_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290391_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:11.46 -02:19:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:39.33 -04:12:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 1.840 3059689076241014272 109.91356328670 -04.21137790261 12.2923 11.8327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290449_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290449_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:58.84 +02:49:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 4.160 3116003450473542784 106.49468568923 +02.82917133305 12.4156 11.5579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290567_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290567_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:43.24 +02:02:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290589_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290589_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:28.46 -00:24:37.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290618_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290618_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:41.63 -00:33:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:12.02 -02:15:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.774 3108852222548310656 105.79942401951 -02.25617766869 12.3669 11.3998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290732_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290732_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:40.36 +01:01:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:29:09.56 -05:33:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290832_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290832_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:21:53.78 +02:20:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290835_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 290835_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290862_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 290862_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:41.26 +00:46:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291022_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291022_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:11.73 -01:59:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291050_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291050_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:21:54.69 +02:22:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291058_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291058_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:00.21 -01:49:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291096_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291096_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:23:43.06 +02:39:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291116_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291116_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:41:37.55 +03:12:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.194 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291139_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291139_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:26:19.64 +01:23:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 2.553 3123455008273752704 096.58153352703 +01.38735719100 12.8884 12.3897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291146_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291146_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:12.75 -04:06:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291228_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291228_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:22:45.49 -02:10:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291242_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291242_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:38.44 +01:13:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291252_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291252_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:08.98 +00:16:36.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291266_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291266_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:42.30 -03:09:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.293 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291324_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291324_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:43.25 -05:30:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291328_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291328_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:21:17.14 -00:11:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 4.170 3121734483032022144 095.32070803228 -00.20016618751 12.9368 12.0752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291333_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291333_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291369_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291369_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291378_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291378_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:18.51 -05:24:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.893 3104187235226900352 096.82605277859 -05.40836792737 12.8062 12.3343 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 291417_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291417_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:03.41 -02:29:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 3.009 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291441_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291441_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291448_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291448_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:23.80 +00:54:09.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291485_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291485_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:18.14 +02:01:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291565_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291565_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:55.17 +00:52:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 3.194 3114390707433383168 107.72973784414 +00.86851239077 12.9930 12.2398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291588_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291588_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:20.80 -05:56:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291601_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291601_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:52.23 +01:55:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291609_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291609_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:48.84 -06:11:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291752_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291752_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291773_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291773_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:52.72 -07:05:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291793_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291793_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291816_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291816_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291862_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291862_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:13.61 +01:34:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.788 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291902_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291902_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:17.55 -04:25:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291909_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291909_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:31:45.02 -05:21:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291924_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 291924_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291930_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 291930_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:29:23.04 +02:43:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292010_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292010_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292032_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292032_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:10.70 -00:39:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.189 3109643252442098176 107.29384914980 -00.65310155480 13.4332 13.0007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:00:51.62 -03:52:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.245 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292049_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292049_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292081_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292081_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292096_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292096_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:24.28 +02:02:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:08.01 -00:13:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.983 3119427535838901376 100.03278128041 -00.22247249061 13.4158 12.5169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292148_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292148_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292150_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292150_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:44.68 -02:33:55.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292177_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292177_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292206_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292206_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292220_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292220_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292238_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292238_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292266_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292266_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:07.45 -01:52:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292279_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292279_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292282_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292282_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292316_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292316_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:12.85 -04:31:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 5.051 3059503293138179072 108.55373641841 -04.53219512048 13.4465 12.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292339_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292339_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292341_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292341_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:43.27 -05:05:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292344_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292344_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:22.54 -03:06:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.558 3108642426286693376 105.34338227084 -03.10135969197 12.9086 11.8972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292359_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292359_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:04.74 +02:28:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292365_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292365_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:20.76 -04:08:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.976 3107624690838876032 107.58557971057 -04.14945019378 13.5191 12.8389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292379_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292379_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292389_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292389_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:25.50 -01:40:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292391_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292391_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292394_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292394_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292405_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292405_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:07.26 +02:40:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292423_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292423_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:19.00 +02:16:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 4.580 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:09.03 +02:20:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292432_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292432_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292437_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292437_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:38.78 +01:32:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292447_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292447_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292498_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292498_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292528_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292528_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292549_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292549_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:22:26.73 -01:42:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.522 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:03.94 +02:09:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292636_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292636_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292640_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292640_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:49.01 -06:01:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292644_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292644_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:55.17 -02:23:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292653_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292653_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:42.19 +00:55:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.818 3123411410063307136 096.17537123953 +00.92203400438 13.4069 12.7060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292661_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292661_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292664_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292664_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:04:51.45 -02:16:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.364 3108857002851931776 106.21398983457 -02.28187184212 13.3926 12.6907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292682_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292682_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:10.32 -02:12:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292700_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292700_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292704_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292704_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:34.73 -01:08:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292715_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292715_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292720_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292720_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:42:39.18 -02:16:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292727_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292727_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292736_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292736_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:48.67 +00:23:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 3.777 3113610294697190784 102.20183118370 +00.39122776001 13.6085 13.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292744_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292744_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:06.99 +01:40:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 5.017 3114693863405107840 106.77860669604 +01.66587278863 13.6698 13.1945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292758_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292758_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:04.59 -05:42:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:10.33 -05:37:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292790_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292790_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292794_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292794_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:55.74 -06:36:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292796_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292796_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:44:11.69 +03:13:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.861 3127311480888772096 101.04831658328 +03.21883456912 13.4524 12.9837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292810_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292810_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:56.29 +01:32:12.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292811_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292811_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:48.75 -02:49:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 5.007 3108008042435350144 106.45202773361 -02.82932879042 13.6288 12.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292813_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292813_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292831_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292831_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292839_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292839_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:58.06 +01:31:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:29:29.78 -00:06:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292879_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292879_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292899_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292899_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:31.30 +00:48:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.471 3111712395887162496 108.88030786344 +00.80659378809 13.6608 12.9499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292913_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292913_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292925_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 292925_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292928_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 292928_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:55.45 -03:46:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293019_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293019_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:39.18 -02:03:03.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293046_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293046_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:19.43 -04:08:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.369 3107624690838875520 107.58011994727 -04.14429608637 13.6473 13.2554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293049_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293049_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:14.77 -02:18:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.538 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293068_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293068_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293069_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293069_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:06.45 +00:05:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293070_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293070_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:45.25 -05:40:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.164 3059140419940666240 107.93738751668 -05.66997036834 13.7391 13.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:22:43.61 -02:10:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293109_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293109_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293110_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293110_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293138_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293138_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:53.39 -03:53:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.617 3107610465908135040 106.72213663188 -03.89031315328 13.6603 13.1510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293152_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293152_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:09.85 +02:55:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293171_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293171_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293174_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293174_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:56:36.59 +02:42:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.000 3127764891995931648 104.15213331048 +02.71143748089 13.6251 13.1744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293188_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293188_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:36.05 +01:59:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293250_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293250_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293251_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293251_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:54.70 +00:45:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.302 3111384127245493376 107.97730601618 +00.76008378136 13.7155 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293293_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293293_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:31:36.96 +00:48:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.201 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293314_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293314_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293316_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293316_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293332_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293332_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:32:12.88 -03:45:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.096 3104990638931443840 098.05302936263 -03.75141229160 13.8715 13.3185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293333_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293333_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:25.30 -03:35:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293334_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293334_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293337_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293337_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293361_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293361_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293362_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293362_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:39:32.32 +03:12:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.589 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293382_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293382_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:58:20.16 -00:33:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.603 3112460446052150272 104.58351260441 -00.55517285309 13.8225 13.3508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293392_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293392_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:53.52 +03:13:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.250 3127291139925000832 100.97237071891 +03.21786171975 13.5859 12.7087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:26.33 -02:20:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.043 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293457_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293457_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293470_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293470_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293481_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:36.98 -04:25:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293484_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293484_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293589_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293589_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293591_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293591_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:37.25 +02:26:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.680 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293616_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293616_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:12.59 -05:08:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293623_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293623_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293627_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293627_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:53.13 +02:30:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.315 3126395102368111488 102.47096542506 +02.50276227856 13.8035 13.2960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293631_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293631_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293633_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293633_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293649_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293649_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:53.15 +01:49:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.699 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293666_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293666_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:59.82 +00:10:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.555 3113319370792412800 103.74872486234 +00.18032112282 13.8383 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293683_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293683_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293690_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293690_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:48.22 -03:44:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.714 3059615374604845824 108.45015657413 -03.73990071395 13.9207 13.6891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293692_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:33.43 +01:51:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.536 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293697_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293697_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:38.70 -00:36:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.179 3109678956510644992 106.66014041170 -00.61650773442 13.7470 12.8165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293703_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293703_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:59.57 -01:03:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.596 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293712_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293712_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293715_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293715_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:41:26.98 -01:19:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293724_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293724_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:55:58.79 -01:35:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.580 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293726_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293726_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293734_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293734_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:42.08 -06:20:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.989 3053036859096886656 107.42497549864 -06.33624383095 12.7148 10.9654 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293741_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293741_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:17.53 -04:07:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.228 3059549129027878528 108.57278260456 -04.13346977507 13.6768 12.9409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293761_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293761_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293764_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293764_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:21.06 -03:11:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293793_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293793_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:12.55 -01:47:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293801_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293801_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293804_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293804_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293805_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293805_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:06.69 +01:33:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.300 3125769140951396608 101.77770849888 +01.56143873464 13.8938 13.1197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:03.63 -03:17:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.892 3060069679063058176 109.76471081547 -03.29241099933 13.9107 13.4866 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 293816_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293816_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293818_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:54:23.06 -02:46:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.384 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293821_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293821_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:20.38 -05:15:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.342 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293855_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293855_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293867_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293869_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:35:42.07 +03:11:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.076 3130161170208610688 098.92490276050 +03.18629758406 13.7622 13.1813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293870_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293881_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293881_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:27.92 -05:57:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.513 3101095172312498048 103.11590743628 -05.95317978863 14.0687 13.5555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293885_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293885_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:22.01 -00:32:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:28.03 -05:15:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.941 3101401729901841408 105.36605808833 -05.25268963173 13.9656 13.5006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293920_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293920_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293927_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293927_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:33.71 -00:26:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.375 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293933_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293933_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293955_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293955_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:16.52 -02:05:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 5.079 3108855903340435200 105.81770007262 -02.09964696229 14.0457 13.5449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 293958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293965_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293965_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:09.51 -05:17:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:54.82 +00:47:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293978_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293978_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:50.84 +01:58:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293989_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293989_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:39:08.74 -03:48:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.748 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 293993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294013_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294013_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:14.86 -04:55:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.928 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294023_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294023_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294043_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294045_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294045_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294054_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294054_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294055_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294055_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294061_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294061_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:29.01 +01:07:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294071_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294071_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294076_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294076_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:13.57 +01:53:01.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294088_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294088_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294090_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294090_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:37:09.75 -01:09:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.480 3118943231029708032 099.29057638008 -01.15179883888 14.0683 13.4931 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 294091_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294091_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294093_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294093_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:37:33.30 +01:24:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.989 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294105_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294105_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:21.09 -05:34:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.100 3101891734129376896 103.08775253888 -05.57718780004 13.3163 12.2056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294113_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294113_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:11.82 +01:54:30.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:02:01.14 -00:33:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 2.430 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294126_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294126_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:44.78 -06:32:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.390 3052268059949126528 107.68596674381 -06.54594956242 14.1177 13.4542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294140_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294140_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:25.29 -00:52:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294143_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:49.78 -06:00:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.685 3100923751580533888 104.95665938724 -06.01033221545 14.0966 13.5643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294144_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294176_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294176_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294178_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294178_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294184_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294184_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:44.04 -05:54:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294187_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294187_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294215_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294215_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294229_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294229_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:41.48 -00:33:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.864 3112503842401083904 103.42233870049 -00.56409058978 14.0403 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294240_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294240_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294242_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294242_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:27.45 -05:52:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294256_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294256_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294268_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294268_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294303_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294303_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:12.09 -02:28:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.363 3108804363733853440 106.30000175483 -02.47624534530 14.0347 13.7941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294308_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294308_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294313_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294313_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294314_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294314_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294322_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294322_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294325_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294325_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294326_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294326_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294334_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294334_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294351_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294351_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294359_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294359_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294366_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294366_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294380_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294380_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294395_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294395_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:35.45 -00:48:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.450 3112578162515589760 105.39724095265 -00.80783877429 14.1459 13.7567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294422_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294422_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294426_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294426_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:34.71 -01:26:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 5.786 3118345204080317440 096.14433564545 -01.44191423101 14.0041 13.5311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294427_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294427_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294435_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294435_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294472_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294472_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:30.80 -05:41:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294495_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294495_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294497_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294497_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:39.53 -00:16:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.463 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294508_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294508_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294515_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294515_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294520_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294520_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294525_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294525_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294563_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294563_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294571_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294571_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:19.84 -04:09:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.462 3107568856264311552 106.58230700457 -04.16288089646 14.2358 13.7444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:14.77 +01:53:13.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294577_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294577_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294583_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294583_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:25:37.50 +01:20:17.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294595_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294595_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:34.31 -01:39:23.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294612_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294612_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:16.48 -04:43:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294665_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294665_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:07.76 +00:56:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.124 3114407371906027008 107.53172595577 +00.94154606542 13.7419 13.0767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294676_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294676_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294695_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294695_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294700_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294700_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294710_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294710_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:38:52.51 +01:12:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294722_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294722_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294747_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294749_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294749_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294753_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294755_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294755_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:26:48.21 +02:38:21.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294778_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294778_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294779_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294779_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294795_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294795_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294806_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294807_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294807_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294812_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294812_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:05.29 -06:32:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294834_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294834_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294841_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294841_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294858_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294858_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:12.16 -01:18:57.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294874_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294874_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294876_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294876_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:30:07.24 -02:39:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.251 3117217616247602048 097.52997534566 -02.66519300427 14.0065 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:24.66 -00:56:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294916_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294916_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294922_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294922_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:59.06 +00:45:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.403 3120401771860646272 096.99561765087 +00.75428578309 14.3945 13.7179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294940_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294940_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294942_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294942_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:19.19 -03:55:33.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294950_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294950_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:53.09 +01:09:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.147 3114472346170617472 106.97045649095 +01.14911711408 13.8927 13.1411 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294953_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294953_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294958_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:37.74 -03:51:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294963_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294963_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:47.47 -07:02:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 3.575 3052741949461733120 105.44720987455 -07.04116892488 14.0487 13.4669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294971_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294971_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:09.61 -02:51:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.622 3105940273380803584 103.28965139707 -02.86233750676 14.0307 13.0420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294978_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294978_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294982_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294982_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:16.27 -01:58:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.319 3109772552442329088 110.06730736101 -01.98023676963 14.1724 13.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294984_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294984_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:10.12 -02:47:56.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294988_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 294988_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:46.00 -02:09:37.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294995_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 294995_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295015_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295015_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:23.66 +01:30:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.433 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295020_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295020_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:29.57 +01:18:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.857 3111661547772738176 109.87300194160 +01.30033766281 14.1404 13.4357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295023_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295023_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295038_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295074_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295074_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:11.56 +01:46:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295078_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295101_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295101_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:58.41 +01:29:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.864 3125767182446332672 101.74323261975 +01.48735629924 14.0034 13.4904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295135_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295135_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:58:20.45 -00:32:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.907 3112460617850838784 104.58465531557 -00.54491251100 14.1966 13.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295139_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295139_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295145_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295145_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295146_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295146_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:29:38.98 +02:15:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.465 3124024181638235520 097.41187370253 +02.26001064907 14.2370 13.5366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295147_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295151_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295151_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:57:28.34 -07:09:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295163_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295163_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:51:34.19 -02:33:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295166_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295166_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:10.10 -06:03:14.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295179_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295179_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295195_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295195_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:52:03.63 -01:41:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.143 3106280434789946240 103.01476275002 -01.69110001977 14.3391 13.5219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295216_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295218_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295218_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295226_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295226_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:08.57 -00:01:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.754 3111232837019910656 107.03525090547 -00.03362767301 14.2683 13.7055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295254_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295254_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295259_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295259_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:14.50 -01:13:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.466 3110074505821408512 109.05984205440 -01.22298851226 14.1401 13.6720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295265_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295265_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:22.43 +01:18:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.669 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295280_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295280_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:29.66 -05:31:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.400 3053331322044768768 106.87363336958 -05.52963771220 14.1610 13.5036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295297_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295297_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295302_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295302_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:14.16 +01:06:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295311_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295311_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:49:38.86 +00:36:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295318_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295318_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295326_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295326_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295343_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295343_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:13.31 +00:50:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.139 3125567827244921728 101.55524044974 +00.83678768778 13.7948 12.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295346_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295346_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:40.78 -00:20:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 5.546 3111162300776365952 107.41991572481 -00.34562381940 14.1693 13.4187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295368_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295368_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:05.17 +02:32:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295397_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295397_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295411_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295411_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295417_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295417_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295439_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295439_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:16.62 -05:04:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.044 3053426017496460416 106.81884344475 -05.08354785989 14.3438 13.5080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295444_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295461_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295461_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295466_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295467_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295467_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:10.44 -01:54:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295506_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:17.99 -04:51:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.449 3059404989926960896 107.82440417551 -04.86285565371 14.2314 13.6329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:00:13.47 -02:20:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 5.551 3108947987437424640 105.05490894300 -02.34750508349 14.2046 13.3405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:22:20.51 -01:14:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.145 3109930847755976064 110.58500365080 -01.23997446257 14.2568 13.6547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295530_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295530_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:05:22.74 -01:37:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.990 3109462966898813184 106.34401149466 -01.61788220358 14.4979 13.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295543_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295543_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295549_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295549_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295556_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295556_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:10.33 -03:48:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295562_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295562_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:14.45 -06:16:31.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295598_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295598_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295600_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295600_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295603_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295603_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:03.07 -06:06:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.627 3053057474940293376 108.01177776358 -06.10169441788 14.3169 13.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295619_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295619_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:01:47.23 -01:24:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.002 3109165140984226176 105.44692959018 -01.41554928022 14.1477 13.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295627_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295627_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295637_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295637_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295639_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295639_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:58.34 -07:05:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295651_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295651_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:36.42 -02:00:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.000 3109751799159544704 109.90133477174 -02.01339188297 14.4137 13.9887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295668_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295668_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295674_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295674_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295701_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295701_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295733_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295733_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295735_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295735_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295750_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295750_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:59.60 -03:18:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.581 3108067072469485568 108.24771270786 -03.30475038064 14.2659 13.7569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295751_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295751_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:18.42 -07:07:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.941 3051951778556709376 109.07595447459 -07.11945308543 14.4378 13.9669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295766_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295774_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295774_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:17.31 -00:43:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.005 3110935006809228800 108.07150437030 -00.72003445389 14.2336 14.0671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295783_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295783_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:44:43.27 -02:06:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.588 3106941413077711360 101.17994342396 -02.10121165387 14.0609 13.1706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295798_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295798_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295811_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295811_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:11.73 +00:43:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.268 3125564734868524928 101.54856583920 +00.72143082097 14.3689 13.4312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295813_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295813_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295822_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295822_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:39.61 -05:23:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.114 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295833_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295833_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295852_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295852_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:46.91 -03:33:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.362 3107672416516031744 108.19477172093 -03.55651695199 14.4535 13.9896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295885_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295885_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:13.94 -04:57:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.448 3053422822040275584 107.05748625646 -04.95736076219 14.2969 13.7887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295903_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295910_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295910_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295918_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295918_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:13.54 +01:07:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295925_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295925_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:38.49 +02:03:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.017 3111964257068274176 109.90952212523 +02.06545282863 14.4750 13.7405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295942_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295942_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:24:07.84 -01:51:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.688 3118222333656012032 096.03204877518 -01.86070191502 14.4257 13.8810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295973_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295973_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:17.92 -03:36:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.266 3107708494242457216 107.32399609933 -03.60153343721 14.5024 14.0580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295974_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295974_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295981_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295981_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:18:18.47 -04:20:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 4.988 3059665024424363520 109.57663726723 -04.34848706095 14.4716 14.0101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295984_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295984_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 295993_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 295995_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 295995_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:48:18.01 +02:45:02.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296003_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296006_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296006_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:32.00 -06:37:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.700 3052231226310118656 108.38261577740 -06.62645481449 14.5620 13.9971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296025_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296025_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296027_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296027_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296037_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296037_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296048_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296065_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296065_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296066_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296066_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296071_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296071_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296077_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296077_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296087_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296087_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296088_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296088_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296093_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296093_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:24.12 -00:37:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.789 3110204488710611968 110.35022641615 -00.62546066998 14.4817 14.1062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296097_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296098_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296098_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:40:26.78 -01:47:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.296 3106835550722792576 100.11111020367 -01.80053406046 14.3775 13.7940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296100_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296100_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:42.20 -00:35:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.576 3112599602992583168 105.92611366219 -00.58925302145 14.4325 13.6354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296109_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296109_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296110_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296110_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296111_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296111_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296114_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296114_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:26.80 +01:30:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.583 3114673694239105408 107.11091176573 +01.50243433392 14.3921 13.6375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296130_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296130_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:11.26 -02:14:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.133 3108254058165525504 109.29652635285 -02.24282967132 14.3544 13.8610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296134_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296136_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296136_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:08.50 -01:15:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.373 3109496746819536512 106.53520082840 -01.26193967133 14.2722 13.4380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296155_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296155_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296160_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296160_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296161_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296161_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296170_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296170_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296172_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296180_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:03.65 +00:02:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.766 3111284033030712960 108.26469190756 +00.04853481648 14.0979 13.0828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296181_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296181_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:02:49.06 -01:46:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.534 3109088175171141632 105.70361971433 -01.77817000677 14.4731 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296191_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296191_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296210_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296210_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296211_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296211_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:28:51.06 +03:09:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296235_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296235_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:46.62 -01:18:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.646 3110091513891011200 108.69346167399 -01.31082750067 14.6235 14.3071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296236_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296236_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296239_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296239_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296243_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:22:12.29 -01:00:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.595 3109990942939026304 110.55133284752 -01.01238137083 14.6172 14.1962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296247_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296256_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296256_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296267_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296267_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:20:25.90 +00:20:49.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296269_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296269_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296287_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296287_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296289_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296289_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296295_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296295_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296310_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296310_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:35.14 -01:01:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.960 3110128725487413120 108.89605821064 -01.02031781928 14.3555 13.8463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296343_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296343_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:11:47.78 +01:41:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.949 3114879509070656640 107.94846133564 +01.69710725632 14.3733 13.5073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296351_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296351_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296362_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296362_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296364_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296364_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296368_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296368_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296380_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296380_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296382_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296382_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296398_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296398_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:15.27 -02:45:44.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296399_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:12.10 -02:20:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.714 3108997293662134400 104.79962658383 -02.33451681197 14.6167 14.2326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296406_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296406_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296410_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:53:47.93 +00:29:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.914 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296424_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296429_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296429_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296440_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296440_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296453_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296453_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:30.96 -00:09:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 4.695 3110996034002383232 108.37792605009 -00.16654559463 14.6766 14.2185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296467_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296467_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:55:32.22 +01:33:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.904 3114123113791161984 103.88347927431 +01.56090348449 14.6417 14.1184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296468_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296468_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:17:55.25 -00:28:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.557 3110257299627475072 109.47935341488 -00.47448920967 14.3401 13.8981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296470_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296470_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:00.94 -02:29:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.372 3108405378450160640 107.25314373552 -02.49393719618 14.0537 13.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296473_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296473_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:14:33.16 -01:27:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.610 3110087596880945536 108.63750355090 -01.45183557752 14.4490 14.0041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296496_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296496_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:47.81 -00:58:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.699 3109417925579939840 107.19868931266 -00.98263679603 14.5970 14.0138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296508_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296508_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:14.47 -02:26:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 4.083 3108411803721141632 107.30972146437 -02.44456392592 14.4345 14.1385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296509_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296509_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296519_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296523_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:15:58.99 -02:16:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.051 3108294843176808576 108.99521570166 -02.27030020588 14.2973 13.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296535_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296535_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296541_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296541_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296542_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296542_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296547_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296547_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296548_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296548_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:07:32.29 -01:29:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.928 3109292787412965504 106.88366036045 -01.48538103804 14.4719 13.6970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296554_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296554_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:35.43 +01:41:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 5.207 3114856041369812992 108.39690518346 +01.69802301952 14.2746 13.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296557_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296557_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:45:04.38 -00:34:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.620 3107448597174462080 101.26781623132 -00.57576830419 14.5378 13.4736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296561_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296561_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:17.37 -01:27:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.387 3108598995575308800 108.07193356417 -01.46276307758 14.3928 13.6951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296566_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296569_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296569_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296573_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296574_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296574_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:10:16.30 -03:45:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.305 3107652831464053248 107.56747719681 -03.76766803909 14.3595 13.6313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296586_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296586_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296588_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296588_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296590_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296590_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:34:48.94 -00:10:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.560 3119662350289897728 098.70332506390 -00.18198105991 14.5966 13.9457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296594_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296594_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:32:48.68 -05:34:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.952 3103428129827401344 098.20246873173 -05.58309149347 14.2179 13.4134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296607_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296607_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296611_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296611_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296612_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296612_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296613_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296616_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296616_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296639_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296639_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:41.09 -03:29:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.668 3107722822252928768 107.17104130651 -03.48881070263 14.5894 14.1660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296643_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296643_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296647_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296647_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:00:02.44 -03:09:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 4.256 3108684894923572480 105.00930760747 -03.15439680797 14.4351 13.6321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296656_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296656_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:08.96 -04:07:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.260 3107534152928192512 107.28726652518 -04.13143194844 14.3172 14.0151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296657_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296657_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:21:13.31 -02:50:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.436 3061608239427210496 110.30496113440 -02.84226658734 14.5231 14.0207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296672_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296672_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296675_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296675_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296681_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296681_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:59:43.71 -02:37:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.584 3108906996270577408 104.93142633250 -02.63195994644 14.3673 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296684_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296684_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296685_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296688_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296688_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296689_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296701_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296701_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:27.90 -02:41:27.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296702_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296702_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:38:10.13 +01:23:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.980 3120638098141033728 099.54150956921 +01.38300044165 14.4812 13.7446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296707_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296707_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:16:51.29 -02:15:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.672 3108254539201896704 109.21349362205 -02.25839110435 14.4496 13.8107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296711_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296711_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:40.66 +01:25:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 5.393 3125752540901542656 101.91906940064 +01.42615378341 14.7186 14.0217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296717_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296717_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:09:41.85 -00:20:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 4.208 3111162300776360704 107.42406179361 -00.34040405718 14.7447 14.2532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296729_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296729_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:25.97 -00:03:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.897 3119489722667709312 100.85767737619 -00.06241890501 14.5999 13.7818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296731_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296749_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296749_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:33:51.93 +03:06:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.496 3130110665691387008 098.46586557876 +03.11355390962 14.5695 13.8418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296757_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296758_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296758_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:13:26.70 +01:02:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.397 3111419071099675264 108.36084362213 +01.03915369488 14.6470 14.1517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296759_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296759_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296761_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296761_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:06:58.92 -04:18:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.818 3107516148424215168 106.74512507633 -04.30121475749 14.3971 13.6185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296764_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296764_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296770_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296770_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296781_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296782_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296782_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296786_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:46:03.34 -03:22:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.701 3105476004593476480 101.51345310619 -03.36958475217 14.7500 14.1257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296794_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296794_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:47:09.12 +02:34:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 4.337 3126465922086428544 101.78759062452 +02.57675584298 14.6202 13.9703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296814_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296814_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296815_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296815_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:09.86 -02:13:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296831_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296831_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296842_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296842_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296859_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296859_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:00:13.39 +02:54:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.609 3115865599202669952 105.05522260708 +02.90651939233 14.6286 14.0643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296861_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296861_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296863_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296863_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:48.64 +00:14:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.424 3119515599849503104 100.95209182411 +00.24630185903 14.6154 14.0717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296871_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296871_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:23:27.12 +02:43:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.260 3124948115002957824 095.86299834490 +02.71714997212 14.4245 13.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296893_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:08:44.98 +00:55:08.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 296904_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:43:24.90 -00:26:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.062 3107445126841047680 100.85351338120 -00.43602507015 14.7791 14.2016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296945_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 296970_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67537_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 67537_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:21:54.92 -04:30:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 65114_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:27:01.37 -04:35:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91187_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 91187_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:29:53.98 -03:35:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 06:50:00.82 +01:46:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.813 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:12:52.18 -05:20:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:19:38.78 -02:00:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-18_21-44-44_20.00sec_-4.90C_LIGHTs_0267 did not pass the final checks
**** FOUND 07:03:53.13 -06:53:23.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 21s
make_report_in_HTML.sh TOTAL: 1310s
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 ####
06:41:43.15 +02:53:01.3
07:09:13.72 -02:21:30.7
07:08:45.34 +00:41:48.8
07:17:31.25 +01:05:39.0
06:51:53.52 +02:07:47.6
06:44:19.75 -00:03:11.7
06:53:51.74 -01:16:59.6
06:44:12.29 -01:09:13.8
06:47:37.26 +01:42:20.5
07:06:26.93 -02:45:27.7
07:05:24.62 -01:37:03.9
06:54:46.97 -00:18:59.5
06:58:00.79 -01:28:24.0
06:45:59.75 +01:38:33.5
06:46:26.75 +00:59:05.0
07:00:32.06 +01:06:04.8
07:02:01.21 +00:39:08.4
07:13:32.71 -00:55:41.4
06:51:22.46 +00:33:45.3
06:55:57.57 +02:33:21.4
06:56:43.24 -02:17:37.5
07:04:18.10 -00:12:34.6
07:05:45.73 -02:32:43.8
06:54:06.97 -01:31:50.2
06:51:18.80 +02:12:27.8
06:37:31.98 +01:46:27.4
06:59:07.03 +00:37:18.7
07:06:13.57 -05:05:05.3
06:56:45.76 -01:04:30.3
06:41:01.89 -01:17:33.8
07:01:53.81 +01:22:52.2
07:04:22.70 +00:59:49.8
07:01:50.23 -01:29:53.3
07:01:18.85 -01:50:06.9
07:09:25.19 -03:13:04.6
06:46:56.80 +01:41:47.9
06:43:22.52 +01:54:52.6
07:11:19.91 -03:51:45.1
07:12:04.38 -02:55:01.6
06:43:46.63 -05:42:06.8
06:58:51.94 +02:39:12.6
07:20:43.53 -02:48:18.5
07:21:21.23 +00:37:45.0
07:00:58.00 -02:15:42.6
06:53:18.48 +01:05:30.6
07:13:39.12 -01:41:16.3
07:15:27.88 -02:44:52.5
07:04:20.04 +02:37:45.2
07:03:37.02 -00:12:38.0
06:56:04.66 -01:29:54.7
07:17:13.61 -02:22:29.0
06:27:15.29 +03:07:46.0
07:19:54.20 -01:00:37.0
06:53:35.64 -01:35:01.5
07:12:39.39 -00:37:46.5
06:49:31.01 +01:58:03.6
07:04:34.81 -03:53:31.6
06:46:31.35 +01:08:38.5
06:29:54.41 +03:09:24.5
06:53:43.61 -01:58:40.8
07:21:19.45 -02:07:51.0
06:54:34.63 -00:15:46.2
07:18:14.13 -05:37:45.6
06:55:40.68 -00:18:33.0
06:56:17.04 +00:50:18.8
06:43:14.62 +01:58:21.4
07:00:46.29 +02:09:09.1
07:19:02.35 -07:07:53.3
07:05:15.99 -05:50:52.5
06:38:28.20 +00:44:36.6
06:46:38.75 +00:42:37.0
07:19:10.42 -01:30:56.3
07:01:34.28 -00:13:23.1
06:43:32.78 +01:24:34.0
06:41:26.78 +02:48:00.9
07:02:32.38 -00:13:08.4
07:12:49.34 -01:30:06.5
06:48:33.32 +01:48:57.5
06:46:10.50 +01:00:20.7
06:37:53.00 -05:55:11.9
06:53:34.07 -00:32:05.1
06:46:25.69 -00:28:35.8
07:19:26.13 +00:51:16.4
06:53:47.01 +01:14:31.6
07:02:52.15 +00:55:00.1
06:46:20.89 +02:44:07.5
07:02:23.51 -01:34:43.4
07:10:10.18 -00:03:45.3
07:09:53.98 -00:44:32.2
07:10:12.62 +01:37:54.7
07:17:36.46 -00:24:01.1
07:18:22.73 +00:37:23.0
07:16:08.24 +00:05:32.3
07:10:10.13 -00:55:09.9
07:15:17.25 -00:21:06.3
07:10:32.61 -05:43:17.1
06:50:11.49 +02:16:28.9
06:54:39.98 +01:28:18.3
07:03:39.79 -04:38:23.8
07:06:31.74 +01:08:40.1
07:20:41.08 -03:34:37.4
07:01:04.17 -04:48:05.7
07:08:57.78 -03:05:11.8
07:01:15.91 +02:06:07.1
07:19:02.10 -06:31:29.9
06:54:39.03 +00:12:16.2
06:30:15.33 +02:16:00.5
07:12:17.29 -02:11:00.1
07:05:20.12 -02:51:44.2
07:09:40.95 -04:22:45.2
07:19:24.04 -02:42:21.0
06:55:07.90 -00:16:28.5
06:44:16.02 -03:32:34.1
07:13:31.49 -03:31:15.0
07:15:56.84 -02:38:27.4
07:09:03.94 -01:19:31.7
06:41:44.27 +00:27:32.2
07:08:21.67 -02:47:08.8
06:54:54.86 -05:37:07.2
06:40:43.75 -01:24:08.9
07:03:25.18 -05:00:40.9
07:07:24.48 +02:31:26.3
07:10:33.35 -03:53:37.9
06:48:07.73 -00:40:39.4
07:09:53.16 -04:01:41.0
06:49:26.81 +02:25:17.1
07:09:41.50 -00:55:18.0
07:11:44.10 -02:16:15.2
06:20:52.80 -06:29:09.0
07:09:57.99 +00:39:43.3
07:06:38.15 -03:18:51.8
06:49:46.90 -00:33:11.0
07:06:31.58 +02:11:38.1
06:51:28.89 +01:57:04.1
06:46:51.22 +02:33:26.9
06:35:07.51 -03:03:03.7
06:51:38.75 +00:29:29.5
06:59:30.47 +00:22:09.3
06:58:50.06 -01:53:08.6
06:43:52.85 +01:17:52.3
07:10:56.75 -04:18:47.4
06:59:00.55 -01:39:58.3
06:58:57.14 -03:00:40.9
07:05:50.92 -02:05:11.4
06:44:31.32 -01:39:34.8
07:10:41.28 -05:05:03.5
07:18:05.05 -01:25:37.6
07:18:41.82 +01:11:02.2
06:59:36.64 +00:07:21.1
06:40:55.32 +00:01:28.0
07:04:15.82 -02:22:56.6
07:03:52.92 +00:49:49.7
06:43:27.90 -03:56:28.1
06:54:34.47 -00:35:22.0
07:07:26.03 -02:04:10.9
07:16:13.34 -00:00:45.0
07:06:44.65 -01:25:53.6
06:50:09.06 +00:56:41.7
06:27:59.03 +02:56:17.9
06:53:11.77 -01:33:37.4
07:17:50.85 -01:41:23.2
06:38:27.90 +00:48:37.4
06:48:15.59 +01:46:16.7
07:08:35.63 +01:46:44.5
06:44:27.39 +02:30:56.5
06:40:30.51 -01:04:41.8
07:00:03.22 -03:18:50.4
07:04:20.46 -02:13:19.9
07:09:20.66 +02:38:45.4
07:17:52.78 +00:17:04.5
07:14:00.02 -02:51:46.6
06:57:16.43 -00:59:39.7
07:05:12.10 -03:19:35.2
07:13:04.82 -05:12:23.7
06:56:02.88 +02:23:22.8
07:09:32.63 -07:02:49.6
06:58:25.52 -02:40:32.3
07:18:20.90 -04:33:02.4
07:09:56.52 -04:34:52.0
06:44:07.44 +03:13:07.3
07:20:03.74 -01:48:50.7
07:04:34.96 -05:56:29.3
07:07:47.05 -02:49:20.6
07:13:59.20 -01:53:59.9
07:18:29.90 -00:11:36.0
07:03:52.72 -06:00:22.1
07:18:50.17 -05:15:14.2
07:22:02.45 +00:44:40.0
07:00:50.76 -00:35:32.2
07:10:37.59 -04:15:17.2
06:58:59.43 -04:37:56.0
07:09:05.02 -02:57:17.9
06:45:57.94 +02:35:25.9
07:05:14.45 +00:02:10.5
07:20:50.53 -00:51:20.8
07:10:06.16 +01:43:43.3
07:03:04.48 -01:18:36.8
07:04:46.61 +02:30:42.1
07:10:18.75 -01:17:09.9
07:04:16.87 -03:01:37.5
07:18:13.69 -00:07:39.7
06:42:33.23 -03:28:05.7
06:44:36.29 +01:45:28.2
07:04:50.40 -01:48:49.9
07:15:26.05 -01:11:22.1
07:18:48.74 -01:43:48.1
07:00:33.81 +02:26:36.6
07:05:47.20 +00:13:23.9
07:06:45.74 -01:30:47.8
06:44:16.60 -00:10:04.5
07:06:45.92 -02:11:02.4
07:04:10.15 -05:04:53.2
07:03:36.84 +02:37:09.8
07:01:14.54 +00:57:28.0
07:07:33.33 -03:25:29.3
06:58:50.18 -04:41:10.7
06:57:12.52 -03:57:43.6
06:30:03.32 +01:18:34.6
06:43:42.42 -04:26:30.3
07:08:04.57 -01:43:40.4
06:35:48.00 +00:35:27.1
07:09:28.93 -06:44:36.9
07:00:38.69 -01:30:47.6
07:02:49.55 -03:11:38.7
06:52:47.86 -06:19:16.6
07:03:07.07 +01:49:30.2
07:06:46.71 -01:31:18.8
07:08:46.29 -02:21:32.3
06:54:39.52 +02:38:02.4
07:14:23.44 -03:02:00.2
07:17:28.58 -01:37:03.7
06:46:51.11 +01:18:12.2
06:43:55.65 -05:03:59.7
07:05:31.89 +02:04:00.7
07:09:14.75 -04:55:03.5
07:08:52.68 -03:55:18.7
06:30:50.32 +02:31:12.6
06:39:05.86 +02:23:36.1
06:26:38.99 +00:26:39.6
06:51:18.33 -01:23:06.9
07:10:24.71 +02:20:19.3
07:03:51.49 -02:54:47.5
06:24:33.54 -01:26:12.8
07:13:48.38 +02:30:37.2
06:44:48.93 +01:46:41.7
07:07:40.35 -03:15:03.6
07:05:35.93 -05:43:55.7
07:01:15.44 -00:32:58.1
07:06:54.26 +02:10:49.8
07:21:49.99 +00:09:23.1
07:03:46.87 -01:04:50.3
06:42:30.97 -06:04:20.5
07:12:41.75 -00:50:01.0
06:57:35.67 +01:13:53.9
07:04:51.68 -02:12:03.7
07:19:27.26 -01:40:46.3
06:45:17.61 +00:43:40.6
06:44:50.83 +01:05:45.3
06:53:02.93 +01:17:29.4
07:05:38.60 +01:26:03.3
06:59:44.43 -01:15:43.0
07:15:43.74 -05:23:23.8
07:10:24.17 -06:40:08.5
07:20:57.72 -02:33:20.3
07:18:39.14 -01:16:48.8
07:04:10.46 -04:42:09.2
07:08:58.19 -02:02:48.7
07:08:43.25 +01:18:05.6
06:45:39.12 +02:45:26.4
07:18:36.19 -02:04:59.2
06:58:22.45 -02:33:50.6
06:49:45.68 +00:30:49.8
06:40:57.09 -04:34:47.9
06:41:21.21 -01:43:16.1
07:07:24.10 -01:20:23.6
07:12:56.48 -03:02:53.3
06:54:26.63 +02:55:34.7
06:37:05.74 +03:07:56.0
07:10:10.81 -02:02:45.9
06:55:19.16 +03:02:04.9
06:58:38.46 -00:18:50.6
06:47:23.79 +01:25:44.9
07:09:31.15 -03:28:26.8
06:46:57.58 -02:12:24.5
07:09:54.20 -04:46:45.0
07:09:21.65 +01:07:27.7
07:20:15.64 -06:40:49.0
06:47:26.83 -04:24:09.2
06:47:12.01 +00:21:20.6
06:58:48.13 -00:36:46.3
06:57:27.64 -05:05:42.1
07:16:37.63 -05:50:18.1
06:59:02.02 +00:56:30.5
07:20:44.76 -05:00:17.0
06:51:36.62 -02:04:10.3
07:09:46.21 -00:21:13.3
06:52:56.87 -04:25:00.4
07:19:50.28 -02:33:24.7
06:53:52.28 -02:12:22.5
06:47:32.89 -01:03:01.2
07:12:26.26 -04:38:59.7
07:11:11.54 -00:11:45.1
06:48:23.32 -05:30:22.9
07:02:37.86 -01:54:03.1
06:50:41.50 -00:31:44.2
06:38:47.12 +02:03:09.6
07:00:20.78 -02:22:07.1
07:08:10.79 -03:12:34.2
07:06:37.06 -01:28:47.0
06:43:53.90 +01:01:54.9
06:38:18.59 -03:21:22.6
06:59:00.99 -02:36:02.6
07:02:55.72 -02:02:36.8
06:48:12.15 -00:18:59.5
06:31:58.75 -03:49:54.8
06:41:21.16 -00:35:21.7
07:05:47.79 +00:29:04.8
06:46:18.44 -02:26:01.1
06:51:28.43 -00:06:28.0
07:08:47.42 -00:37:49.3
07:04:40.36 -01:02:13.7
06:38:32.13 +02:21:50.6
06:56:37.89 +00:11:26.0
06:32:57.59 -02:23:11.8
07:14:42.78 -02:55:32.3
07:05:05.62 +02:17:06.7
06:55:34.59 +01:52:30.2
06:47:10.53 +02:54:04.4
07:21:37.13 +02:27:48.5
07:11:24.98 -05:58:01.4
06:45:54.15 -00:09:36.4
06:54:01.69 -02:07:17.0
07:07:15.74 +02:06:37.0
06:38:15.57 +00:43:52.6
06:51:24.01 +00:52:45.8
06:56:41.81 -00:14:41.1
06:53:39.64 +00:03:18.3
07:00:12.27 -01:50:10.3
07:12:49.07 -03:33:13.0
06:58:34.56 -01:38:22.8
06:55:50.76 -02:12:27.4
06:38:37.28 -02:20:02.8
06:56:31.80 +02:40:02.5
07:11:22.90 -03:40:07.3
06:57:32.77 -05:57:35.7
06:40:47.22 -01:31:42.0
06:44:36.38 -00:34:40.8
07:13:09.03 +02:42:09.3
06:59:18.34 +02:00:31.3
06:51:11.58 -02:22:08.9
07:07:29.49 +01:15:34.1
07:21:08.26 -01:43:14.9
06:20:28.15 -03:16:34.6
06:55:46.11 +00:37:44.4
07:11:46.28 +01:10:54.4
07:09:19.51 -00:22:15.1
07:09:25.87 -02:13:07.3
06:58:11.17 -02:26:27.3
06:50:55.39 -01:20:54.8
06:52:15.51 -01:19:38.7
07:00:32.43 -03:26:18.3
07:09:37.91 -00:01:16.9
07:01:45.48 -00:36:23.3
07:19:23.84 +00:34:10.6
06:48:04.27 -01:54:51.4
07:07:16.70 +01:31:11.8
07:04:19.83 +00:50:07.3
06:56:25.52 -03:54:41.1
07:05:44.24 -02:20:49.5
06:24:14.93 +00:04:42.4
06:26:19.97 -00:45:06.8
07:03:50.85 -01:11:02.4
06:55:03.30 +01:21:34.7
06:42:39.85 +01:17:02.6
06:56:06.42 -04:22:09.2
07:05:41.38 -03:03:49.3
06:45:15.40 -00:22:56.5
07:20:06.00 -02:24:28.4
07:03:44.53 -02:34:43.9
06:46:37.95 +02:08:17.8
06:30:03.84 -01:08:31.7
06:57:58.69 -05:42:47.1
07:10:48.74 -05:12:39.3
07:07:21.15 +00:33:34.9
06:51:46.23 +02:39:47.7
07:07:11.77 -02:35:01.6
07:12:42.54 -04:10:12.5
07:19:12.60 -01:22:35.5
07:01:15.43 -05:20:34.3
07:18:32.61 -01:20:52.4
07:18:52.05 -03:35:10.6
07:09:40.33 -02:29:08.6
06:46:04.24 -02:35:17.2
07:01:56.05 +01:13:08.5
06:54:09.36 +01:41:25.2
06:41:04.21 +02:37:12.2
07:12:49.59 -00:29:11.3
06:55:56.32 +02:39:57.1
07:19:52.56 +00:18:03.9
06:48:44.11 +02:30:00.2
07:03:53.59 +01:24:55.8
07:19:04.11 +00:51:17.9
07:12:45.14 +01:18:47.2
07:01:12.84 -03:51:27.8
06:57:20.23 -01:46:09.4
07:03:48.73 -01:24:40.5
06:39:06.21 +00:32:11.4
07:12:23.96 -02:24:26.6
07:10:31.33 -00:55:56.3
07:02:28.55 +02:29:05.2
07:06:40.26 +00:42:28.4
06:54:13.65 +02:59:21.4
06:36:38.11 -00:15:14.8
06:52:19.06 +00:50:21.6
06:56:18.54 -02:55:33.0
07:12:18.57 -03:48:49.1
06:57:56.59 -02:44:53.0
06:57:19.64 -02:37:56.7
06:54:40.17 -00:46:47.9
07:01:14.59 +01:01:15.8
06:53:03.14 -00:27:34.5
06:45:14.28 -01:50:55.9
07:17:27.14 -00:59:54.5
07:02:55.58 +02:43:40.0
06:59:50.28 -01:50:11.7
07:00:23.20 +00:26:32.7
06:48:40.33 -01:40:12.9
06:30:11.45 +01:52:29.9
07:22:26.05 +00:56:45.9
07:19:10.41 -01:27:06.6
07:02:53.40 -01:36:00.2
07:08:53.87 +00:51:37.1
06:52:30.57 -02:40:20.2
06:59:26.22 -00:40:38.3
07:09:39.99 +01:41:30.4
06:45:28.49 +01:05:23.4
06:47:34.69 +02:44:50.8
06:45:45.32 +01:55:47.1
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:41:43.15 +02:53:01.3
06:51:53.52 +02:07:47.6
06:44:19.75 -00:03:11.7
06:53:51.74 -01:16:59.6
06:44:12.29 -01:09:13.8
06:47:37.26 +01:42:20.5
07:06:26.93 -02:45:27.7
07:05:24.62 -01:37:03.9
06:54:46.97 -00:18:59.5
06:58:00.79 -01:28:24.0
06:45:59.75 +01:38:33.5
06:46:26.75 +00:59:05.0
07:00:32.06 +01:06:04.8
07:02:01.21 +00:39:08.4
07:13:32.71 -00:55:41.4
06:51:22.46 +00:33:45.3
06:55:57.57 +02:33:21.4
06:56:43.24 -02:17:37.5
07:04:18.10 -00:12:34.6
07:05:45.73 -02:32:43.8
06:54:06.97 -01:31:50.2
06:51:18.80 +02:12:27.8
06:37:31.98 +01:46:27.4
06:59:07.03 +00:37:18.7
07:06:13.57 -05:05:05.3
06:56:45.76 -01:04:30.3
06:41:01.89 -01:17:33.8
07:01:53.81 +01:22:52.2
07:04:22.70 +00:59:49.8
07:01:50.23 -01:29:53.3
07:01:18.85 -01:50:06.9
07:09:25.19 -03:13:04.6
06:46:56.80 +01:41:47.9
06:43:22.52 +01:54:52.6
07:11:19.91 -03:51:45.1
07:12:04.38 -02:55:01.6
06:43:46.63 -05:42:06.8
06:58:51.94 +02:39:12.6
07:20:43.53 -02:48:18.5
07:21:21.23 +00:37:45.0
07:00:58.00 -02:15:42.6
06:53:18.48 +01:05:30.6
07:13:39.12 -01:41:16.3
07:15:27.88 -02:44:52.5
07:04:20.04 +02:37:45.2
07:03:37.02 -00:12:38.0
06:56:04.66 -01:29:54.7
07:17:13.61 -02:22:29.0
06:27:15.29 +03:07:46.0
07:19:54.20 -01:00:37.0
06:53:35.64 -01:35:01.5
07:12:39.39 -00:37:46.5
06:49:31.01 +01:58:03.6
07:04:34.81 -03:53:31.6
06:46:31.35 +01:08:38.5
06:29:54.41 +03:09:24.5
06:53:43.61 -01:58:40.8
07:21:19.45 -02:07:51.0
06:54:34.63 -00:15:46.2
07:18:14.13 -05:37:45.6
06:55:40.68 -00:18:33.0
06:56:17.04 +00:50:18.8
06:43:14.62 +01:58:21.4
07:00:46.29 +02:09:09.1
07:19:02.35 -07:07:53.3
07:05:15.99 -05:50:52.5
06:38:28.20 +00:44:36.6
06:46:38.75 +00:42:37.0
07:19:10.42 -01:30:56.3
07:01:34.28 -00:13:23.1
06:43:32.78 +01:24:34.0
06:41:26.78 +02:48:00.9
07:02:32.38 -00:13:08.4
07:12:49.34 -01:30:06.5
06:48:33.32 +01:48:57.5
06:46:10.50 +01:00:20.7
06:37:53.00 -05:55:11.9
06:53:34.07 -00:32:05.1
06:46:25.69 -00:28:35.8
07:19:26.13 +00:51:16.4
06:53:47.01 +01:14:31.6
07:02:52.15 +00:55:00.1
06:46:20.89 +02:44:07.5
07:02:23.51 -01:34:43.4
07:10:10.18 -00:03:45.3
07:09:53.98 -00:44:32.2
07:10:12.62 +01:37:54.7
07:17:36.46 -00:24:01.1
07:18:22.73 +00:37:23.0
07:16:08.24 +00:05:32.3
07:10:10.13 -00:55:09.9
07:15:17.25 -00:21:06.3
07:10:32.61 -05:43:17.1
06:50:11.49 +02:16:28.9
06:54:39.98 +01:28:18.3
07:03:39.79 -04:38:23.8
07:06:31.74 +01:08:40.1
07:20:41.08 -03:34:37.4
07:01:04.17 -04:48:05.7
07:08:57.78 -03:05:11.8
07:01:15.91 +02:06:07.1
07:19:02.10 -06:31:29.9
06:54:39.03 +00:12:16.2
06:30:15.33 +02:16:00.5
07:12:17.29 -02:11:00.1
07:05:20.12 -02:51:44.2
07:09:40.95 -04:22:45.2
07:19:24.04 -02:42:21.0
06:55:07.90 -00:16:28.5
06:44:16.02 -03:32:34.1
07:13:31.49 -03:31:15.0
07:15:56.84 -02:38:27.4
07:09:03.94 -01:19:31.7
06:41:44.27 +00:27:32.2
07:08:21.67 -02:47:08.8
06:54:54.86 -05:37:07.2
06:40:43.75 -01:24:08.9
07:03:25.18 -05:00:40.9
07:07:24.48 +02:31:26.3
07:10:33.35 -03:53:37.9
06:48:07.73 -00:40:39.4
07:09:53.16 -04:01:41.0
06:49:26.81 +02:25:17.1
07:09:41.50 -00:55:18.0
07:11:44.10 -02:16:15.2
06:20:52.80 -06:29:09.0
07:09:57.99 +00:39:43.3
07:06:38.15 -03:18:51.8
06:49:46.90 -00:33:11.0
07:06:31.58 +02:11:38.1
06:51:28.89 +01:57:04.1
06:46:51.22 +02:33:26.9
06:35:07.51 -03:03:03.7
06:51:38.75 +00:29:29.5
06:59:30.47 +00:22:09.3
06:58:50.06 -01:53:08.6
06:43:52.85 +01:17:52.3
07:10:56.75 -04:18:47.4
06:59:00.55 -01:39:58.3
06:58:57.14 -03:00:40.9
07:05:50.92 -02:05:11.4
06:44:31.32 -01:39:34.8
07:10:41.28 -05:05:03.5
07:18:05.05 -01:25:37.6
07:18:41.82 +01:11:02.2
06:59:36.64 +00:07:21.1
06:40:55.32 +00:01:28.0
07:04:15.82 -02:22:56.6
07:03:52.92 +00:49:49.7
06:43:27.90 -03:56:28.1
06:54:34.47 -00:35:22.0
07:07:26.03 -02:04:10.9
07:16:13.34 -00:00:45.0
07:06:44.65 -01:25:53.6
06:50:09.06 +00:56:41.7
06:27:59.03 +02:56:17.9
06:53:11.77 -01:33:37.4
07:17:50.85 -01:41:23.2
06:38:27.90 +00:48:37.4
06:48:15.59 +01:46:16.7
07:08:35.63 +01:46:44.5
06:44:27.39 +02:30:56.5
06:40:30.51 -01:04:41.8
07:00:03.22 -03:18:50.4
07:04:20.46 -02:13:19.9
07:09:20.66 +02:38:45.4
07:17:52.78 +00:17:04.5
07:14:00.02 -02:51:46.6
06:57:16.43 -00:59:39.7
07:05:12.10 -03:19:35.2
07:13:04.82 -05:12:23.7
06:56:02.88 +02:23:22.8
07:09:32.63 -07:02:49.6
06:58:25.52 -02:40:32.3
07:18:20.90 -04:33:02.4
07:09:56.52 -04:34:52.0
06:44:07.44 +03:13:07.3
07:20:03.74 -01:48:50.7
07:04:34.96 -05:56:29.3
07:07:47.05 -02:49:20.6
07:13:59.20 -01:53:59.9
07:18:29.90 -00:11:36.0
07:03:52.72 -06:00:22.1
07:18:50.17 -05:15:14.2
07:22:02.45 +00:44:40.0
07:00:50.76 -00:35:32.2
07:10:37.59 -04:15:17.2
06:58:59.43 -04:37:56.0
07:09:05.02 -02:57:17.9
06:45:57.94 +02:35:25.9
07:05:14.45 +00:02:10.5
07:20:50.53 -00:51:20.8
07:10:06.16 +01:43:43.3
07:03:04.48 -01:18:36.8
07:04:46.61 +02:30:42.1
07:10:18.75 -01:17:09.9
07:04:16.87 -03:01:37.5
07:18:13.69 -00:07:39.7
06:42:33.23 -03:28:05.7
06:44:36.29 +01:45:28.2
07:04:50.40 -01:48:49.9
07:15:26.05 -01:11:22.1
07:18:48.74 -01:43:48.1
07:00:33.81 +02:26:36.6
07:05:47.20 +00:13:23.9
07:06:45.74 -01:30:47.8
06:44:16.60 -00:10:04.5
07:06:45.92 -02:11:02.4
07:04:10.15 -05:04:53.2
07:03:36.84 +02:37:09.8
07:01:14.54 +00:57:28.0
07:07:33.33 -03:25:29.3
06:58:50.18 -04:41:10.7
06:57:12.52 -03:57:43.6
06:30:03.32 +01:18:34.6
06:43:42.42 -04:26:30.3
07:08:04.57 -01:43:40.4
06:35:48.00 +00:35:27.1
07:09:28.93 -06:44:36.9
07:00:38.69 -01:30:47.6
07:02:49.55 -03:11:38.7
06:52:47.86 -06:19:16.6
07:03:07.07 +01:49:30.2
07:06:46.71 -01:31:18.8
07:08:46.29 -02:21:32.3
06:54:39.52 +02:38:02.4
07:14:23.44 -03:02:00.2
07:17:28.58 -01:37:03.7
06:46:51.11 +01:18:12.2
06:43:55.65 -05:03:59.7
07:05:31.89 +02:04:00.7
07:09:14.75 -04:55:03.5
07:08:52.68 -03:55:18.7
06:30:50.32 +02:31:12.6
06:39:05.86 +02:23:36.1
06:26:38.99 +00:26:39.6
06:51:18.33 -01:23:06.9
07:10:24.71 +02:20:19.3
07:03:51.49 -02:54:47.5
06:24:33.54 -01:26:12.8
07:13:48.38 +02:30:37.2
06:44:48.93 +01:46:41.7
07:07:40.35 -03:15:03.6
07:05:35.93 -05:43:55.7
07:01:15.44 -00:32:58.1
07:06:54.26 +02:10:49.8
07:21:49.99 +00:09:23.1
07:03:46.87 -01:04:50.3
06:42:30.97 -06:04:20.5
07:12:41.75 -00:50:01.0
06:57:35.67 +01:13:53.9
07:04:51.68 -02:12:03.7
07:19:27.26 -01:40:46.3
06:45:17.61 +00:43:40.6
06:44:50.83 +01:05:45.3
06:53:02.93 +01:17:29.4
07:05:38.60 +01:26:03.3
06:59:44.43 -01:15:43.0
07:15:43.74 -05:23:23.8
07:10:24.17 -06:40:08.5
07:20:57.72 -02:33:20.3
07:18:39.14 -01:16:48.8
07:04:10.46 -04:42:09.2
07:08:58.19 -02:02:48.7
07:08:43.25 +01:18:05.6
06:45:39.12 +02:45:26.4
07:18:36.19 -02:04:59.2
06:58:22.45 -02:33:50.6
06:49:45.68 +00:30:49.8
06:40:57.09 -04:34:47.9
06:41:21.21 -01:43:16.1
07:07:24.10 -01:20:23.6
07:12:56.48 -03:02:53.3
06:54:26.63 +02:55:34.7
06:37:05.74 +03:07:56.0
07:10:10.81 -02:02:45.9
06:55:19.16 +03:02:04.9
06:58:38.46 -00:18:50.6
06:47:23.79 +01:25:44.9
07:09:31.15 -03:28:26.8
06:46:57.58 -02:12:24.5
07:09:54.20 -04:46:45.0
07:09:21.65 +01:07:27.7
07:20:15.64 -06:40:49.0
06:47:26.83 -04:24:09.2
06:47:12.01 +00:21:20.6
06:58:48.13 -00:36:46.3
06:57:27.64 -05:05:42.1
07:16:37.63 -05:50:18.1
06:59:02.02 +00:56:30.5
07:20:44.76 -05:00:17.0
06:51:36.62 -02:04:10.3
07:09:46.21 -00:21:13.3
06:52:56.87 -04:25:00.4
07:19:50.28 -02:33:24.7
06:53:52.28 -02:12:22.5
06:47:32.89 -01:03:01.2
07:12:26.26 -04:38:59.7
07:11:11.54 -00:11:45.1
06:48:23.32 -05:30:22.9
07:02:37.86 -01:54:03.1
06:50:41.50 -00:31:44.2
06:38:47.12 +02:03:09.6
07:00:20.78 -02:22:07.1
07:08:10.79 -03:12:34.2
07:06:37.06 -01:28:47.0
06:43:53.90 +01:01:54.9
06:38:18.59 -03:21:22.6
06:59:00.99 -02:36:02.6
07:02:55.72 -02:02:36.8
06:48:12.15 -00:18:59.5
06:31:58.75 -03:49:54.8
06:41:21.16 -00:35:21.7
07:05:47.79 +00:29:04.8
06:46:18.44 -02:26:01.1
06:51:28.43 -00:06:28.0
07:08:47.42 -00:37:49.3
07:04:40.36 -01:02:13.7
06:38:32.13 +02:21:50.6
06:56:37.89 +00:11:26.0
06:32:57.59 -02:23:11.8
07:14:42.78 -02:55:32.3
07:05:05.62 +02:17:06.7
06:55:34.59 +01:52:30.2
06:47:10.53 +02:54:04.4
07:21:37.13 +02:27:48.5
07:11:24.98 -05:58:01.4
06:45:54.15 -00:09:36.4
06:54:01.69 -02:07:17.0
07:07:15.74 +02:06:37.0
06:38:15.57 +00:43:52.6
06:51:24.01 +00:52:45.8
06:56:41.81 -00:14:41.1
06:53:39.64 +00:03:18.3
07:00:12.27 -01:50:10.3
07:12:49.07 -03:33:13.0
06:58:34.56 -01:38:22.8
06:55:50.76 -02:12:27.4
06:38:37.28 -02:20:02.8
06:56:31.80 +02:40:02.5
07:11:22.90 -03:40:07.3
06:57:32.77 -05:57:35.7
06:40:47.22 -01:31:42.0
06:44:36.38 -00:34:40.8
07:13:09.03 +02:42:09.3
06:59:18.34 +02:00:31.3
06:51:11.58 -02:22:08.9
07:07:29.49 +01:15:34.1
07:21:08.26 -01:43:14.9
06:20:28.15 -03:16:34.6
06:55:46.11 +00:37:44.4
07:11:46.28 +01:10:54.4
07:09:19.51 -00:22:15.1
07:09:25.87 -02:13:07.3
06:58:11.17 -02:26:27.3
06:50:55.39 -01:20:54.8
06:52:15.51 -01:19:38.7
07:00:32.43 -03:26:18.3
07:09:37.91 -00:01:16.9
07:01:45.48 -00:36:23.3
07:19:23.84 +00:34:10.6
06:48:04.27 -01:54:51.4
07:07:16.70 +01:31:11.8
07:04:19.83 +00:50:07.3
06:56:25.52 -03:54:41.1
07:05:44.24 -02:20:49.5
06:24:14.93 +00:04:42.4
06:26:19.97 -00:45:06.8
07:03:50.85 -01:11:02.4
06:55:03.30 +01:21:34.7
06:42:39.85 +01:17:02.6
06:56:06.42 -04:22:09.2
07:05:41.38 -03:03:49.3
06:45:15.40 -00:22:56.5
07:20:06.00 -02:24:28.4
07:03:44.53 -02:34:43.9
06:46:37.95 +02:08:17.8
06:30:03.84 -01:08:31.7
06:57:58.69 -05:42:47.1
07:10:48.74 -05:12:39.3
07:07:21.15 +00:33:34.9
06:51:46.23 +02:39:47.7
07:07:11.77 -02:35:01.6
07:12:42.54 -04:10:12.5
07:19:12.60 -01:22:35.5
07:01:15.43 -05:20:34.3
07:18:32.61 -01:20:52.4
07:18:52.05 -03:35:10.6
07:09:40.33 -02:29:08.6
06:46:04.24 -02:35:17.2
07:01:56.05 +01:13:08.5
06:54:09.36 +01:41:25.2
06:41:04.21 +02:37:12.2
07:12:49.59 -00:29:11.3
06:55:56.32 +02:39:57.1
07:19:52.56 +00:18:03.9
06:48:44.11 +02:30:00.2
07:03:53.59 +01:24:55.8
07:19:04.11 +00:51:17.9
07:12:45.14 +01:18:47.2
07:01:12.84 -03:51:27.8
06:57:20.23 -01:46:09.4
07:03:48.73 -01:24:40.5
06:39:06.21 +00:32:11.4
07:12:23.96 -02:24:26.6
07:10:31.33 -00:55:56.3
07:02:28.55 +02:29:05.2
07:06:40.26 +00:42:28.4
06:54:13.65 +02:59:21.4
06:36:38.11 -00:15:14.8
06:52:19.06 +00:50:21.6
06:56:18.54 -02:55:33.0
07:12:18.57 -03:48:49.1
06:57:56.59 -02:44:53.0
06:57:19.64 -02:37:56.7
06:54:40.17 -00:46:47.9
07:01:14.59 +01:01:15.8
06:53:03.14 -00:27:34.5
06:45:14.28 -01:50:55.9
07:17:27.14 -00:59:54.5
07:02:55.58 +02:43:40.0
06:59:50.28 -01:50:11.7
07:00:23.20 +00:26:32.7
06:48:40.33 -01:40:12.9
06:30:11.45 +01:52:29.9
07:22:26.05 +00:56:45.9
07:19:10.41 -01:27:06.6
07:02:53.40 -01:36:00.2
07:08:53.87 +00:51:37.1
06:52:30.57 -02:40:20.2
06:59:26.22 -00:40:38.3
07:09:39.99 +01:41:30.4
06:45:28.49 +01:05:23.4
06:47:34.69 +02:44:50.8
06:45:45.32 +01:55:47.1
07:09:13.72 -02:21:30.7
07:08:45.34 +00:41:48.8
07:17:31.25 +01:05:39.0
###################################################################################
06:41:43.15 +02:53:01.3 -- not an asteroid (will add it to exclusion list)
06:51:53.52 +02:07:47.6 -- not an asteroid (will add it to exclusion list)
06:44:19.75 -00:03:11.7 -- not an asteroid (will add it to exclusion list)
06:53:51.74 -01:16:59.6 -- not an asteroid (will add it to exclusion list)
06:44:12.29 -01:09:13.8 -- not an asteroid (will add it to exclusion list)
06:47:37.26 +01:42:20.5 -- not an asteroid (will add it to exclusion list)
07:06:26.93 -02:45:27.7 -- not an asteroid (will add it to exclusion list)
07:05:24.62 -01:37:03.9 -- not an asteroid (will add it to exclusion list)
06:54:46.97 -00:18:59.5 -- not an asteroid (will add it to exclusion list)
06:58:00.79 -01:28:24.0 -- not an asteroid (will add it to exclusion list)
06:45:59.75 +01:38:33.5 -- not an asteroid (will add it to exclusion list)
06:46:26.75 +00:59:05.0 -- not an asteroid (will add it to exclusion list)
07:00:32.06 +01:06:04.8 -- not an asteroid (will add it to exclusion list)
07:02:01.21 +00:39:08.4 -- not an asteroid (will add it to exclusion list)
07:13:32.71 -00:55:41.4 -- not an asteroid (will add it to exclusion list)
06:51:22.46 +00:33:45.3 -- not an asteroid (will add it to exclusion list)
06:55:57.57 +02:33:21.4 -- not an asteroid (will add it to exclusion list)
06:56:43.24 -02:17:37.5 -- not an asteroid (will add it to exclusion list)
07:04:18.10 -00:12:34.6 -- not an asteroid (will add it to exclusion list)
07:05:45.73 -02:32:43.8 -- not an asteroid (will add it to exclusion list)
06:54:06.97 -01:31:50.2 -- not an asteroid (will add it to exclusion list)
06:51:18.80 +02:12:27.8 -- not an asteroid (will add it to exclusion list)
06:37:31.98 +01:46:27.4 -- not an asteroid (will add it to exclusion list)
06:59:07.03 +00:37:18.7 -- not an asteroid (will add it to exclusion list)
07:06:13.57 -05:05:05.3 -- not an asteroid (will add it to exclusion list)
06:56:45.76 -01:04:30.3 -- not an asteroid (will add it to exclusion list)
06:41:01.89 -01:17:33.8 -- not an asteroid (will add it to exclusion list)
07:01:53.81 +01:22:52.2 -- not an asteroid (will add it to exclusion list)
07:04:22.70 +00:59:49.8 -- not an asteroid (will add it to exclusion list)
07:01:50.23 -01:29:53.3 -- not an asteroid (will add it to exclusion list)
07:01:18.85 -01:50:06.9 -- not an asteroid (will add it to exclusion list)
07:09:25.19 -03:13:04.6 -- not an asteroid (will add it to exclusion list)
06:46:56.80 +01:41:47.9 -- not an asteroid (will add it to exclusion list)
06:43:22.52 +01:54:52.6 -- not an asteroid (will add it to exclusion list)
07:11:19.91 -03:51:45.1 -- not an asteroid (will add it to exclusion list)
07:12:04.38 -02:55:01.6 -- not an asteroid (will add it to exclusion list)
06:43:46.63 -05:42:06.8 -- not an asteroid (will add it to exclusion list)
06:58:51.94 +02:39:12.6 -- not an asteroid (will add it to exclusion list)
07:20:43.53 -02:48:18.5 -- not an asteroid (will add it to exclusion list)
07:21:21.23 +00:37:45.0 -- not an asteroid (will add it to exclusion list)
07:00:58.00 -02:15:42.6 -- not an asteroid (will add it to exclusion list)
06:53:18.48 +01:05:30.6 -- not an asteroid (will add it to exclusion list)
07:13:39.12 -01:41:16.3 -- not an asteroid (will add it to exclusion list)
07:15:27.88 -02:44:52.5 -- not an asteroid (will add it to exclusion list)
07:04:20.04 +02:37:45.2 -- not an asteroid (will add it to exclusion list)
07:03:37.02 -00:12:38.0 -- not an asteroid (will add it to exclusion list)
06:56:04.66 -01:29:54.7 -- not an asteroid (will add it to exclusion list)
07:17:13.61 -02:22:29.0 -- not an asteroid (will add it to exclusion list)
06:27:15.29 +03:07:46.0 -- not an asteroid (will add it to exclusion list)
07:19:54.20 -01:00:37.0 -- not an asteroid (will add it to exclusion list)
06:53:35.64 -01:35:01.5 -- not an asteroid (will add it to exclusion list)
07:12:39.39 -00:37:46.5 -- not an asteroid (will add it to exclusion list)
06:49:31.01 +01:58:03.6 -- not an asteroid (will add it to exclusion list)
07:04:34.81 -03:53:31.6 -- not an asteroid (will add it to exclusion list)
06:46:31.35 +01:08:38.5 -- not an asteroid (will add it to exclusion list)
06:29:54.41 +03:09:24.5 -- not an asteroid (will add it to exclusion list)
06:53:43.61 -01:58:40.8 -- not an asteroid (will add it to exclusion list)
07:21:19.45 -02:07:51.0 -- not an asteroid (will add it to exclusion list)
06:54:34.63 -00:15:46.2 -- not an asteroid (will add it to exclusion list)
07:18:14.13 -05:37:45.6 -- not an asteroid (will add it to exclusion list)
06:55:40.68 -00:18:33.0 -- not an asteroid (will add it to exclusion list)
06:56:17.04 +00:50:18.8 -- not an asteroid (will add it to exclusion list)
06:43:14.62 +01:58:21.4 -- not an asteroid (will add it to exclusion list)
07:00:46.29 +02:09:09.1 -- not an asteroid (will add it to exclusion list)
07:19:02.35 -07:07:53.3 -- not an asteroid (will add it to exclusion list)
07:05:15.99 -05:50:52.5 -- not an asteroid (will add it to exclusion list)
06:38:28.20 +00:44:36.6 -- not an asteroid (will add it to exclusion list)
06:46:38.75 +00:42:37.0 -- not an asteroid (will add it to exclusion list)
07:19:10.42 -01:30:56.3 -- not an asteroid (will add it to exclusion list)
07:01:34.28 -00:13:23.1 -- not an asteroid (will add it to exclusion list)
06:43:32.78 +01:24:34.0 -- not an asteroid (will add it to exclusion list)
06:41:26.78 +02:48:00.9 -- not an asteroid (will add it to exclusion list)
07:02:32.38 -00:13:08.4 -- not an asteroid (will add it to exclusion list)
07:12:49.34 -01:30:06.5 -- not an asteroid (will add it to exclusion list)
06:48:33.32 +01:48:57.5 -- not an asteroid (will add it to exclusion list)
06:46:10.50 +01:00:20.7 -- not an asteroid (will add it to exclusion list)
06:37:53.00 -05:55:11.9 -- not an asteroid (will add it to exclusion list)
06:53:34.07 -00:32:05.1 -- not an asteroid (will add it to exclusion list)
06:46:25.69 -00:28:35.8 -- not an asteroid (will add it to exclusion list)
07:19:26.13 +00:51:16.4 -- not an asteroid (will add it to exclusion list)
06:53:47.01 +01:14:31.6 -- not an asteroid (will add it to exclusion list)
07:02:52.15 +00:55:00.1 -- not an asteroid (will add it to exclusion list)
06:46:20.89 +02:44:07.5 -- not an asteroid (will add it to exclusion list)
07:02:23.51 -01:34:43.4 -- not an asteroid (will add it to exclusion list)
07:10:10.18 -00:03:45.3 -- not an asteroid (will add it to exclusion list)
07:09:53.98 -00:44:32.2 -- not an asteroid (will add it to exclusion list)
07:10:12.62 +01:37:54.7 -- not an asteroid (will add it to exclusion list)
07:17:36.46 -00:24:01.1 -- not an asteroid (will add it to exclusion list)
07:18:22.73 +00:37:23.0 -- not an asteroid (will add it to exclusion list)
07:16:08.24 +00:05:32.3 -- not an asteroid (will add it to exclusion list)
07:10:10.13 -00:55:09.9 -- not an asteroid (will add it to exclusion list)
07:15:17.25 -00:21:06.3 -- not an asteroid (will add it to exclusion list)
07:10:32.61 -05:43:17.1 -- not an asteroid (will add it to exclusion list)
06:50:11.49 +02:16:28.9 -- not an asteroid (will add it to exclusion list)
06:54:39.98 +01:28:18.3 -- not an asteroid (will add it to exclusion list)
07:03:39.79 -04:38:23.8 -- not an asteroid (will add it to exclusion list)
07:06:31.74 +01:08:40.1 -- not an asteroid (will add it to exclusion list)
07:20:41.08 -03:34:37.4 -- not an asteroid (will add it to exclusion list)
07:01:04.17 -04:48:05.7 -- not an asteroid (will add it to exclusion list)
07:08:57.78 -03:05:11.8 -- not an asteroid (will add it to exclusion list)
07:01:15.91 +02:06:07.1 -- not an asteroid (will add it to exclusion list)
07:19:02.10 -06:31:29.9 -- not an asteroid (will add it to exclusion list)
06:54:39.03 +00:12:16.2 -- not an asteroid (will add it to exclusion list)
06:30:15.33 +02:16:00.5 -- not an asteroid (will add it to exclusion list)
07:12:17.29 -02:11:00.1 -- not an asteroid (will add it to exclusion list)
07:05:20.12 -02:51:44.2 -- not an asteroid (will add it to exclusion list)
07:09:40.95 -04:22:45.2 -- not an asteroid (will add it to exclusion list)
07:19:24.04 -02:42:21.0 -- not an asteroid (will add it to exclusion list)
06:55:07.90 -00:16:28.5 -- not an asteroid (will add it to exclusion list)
06:44:16.02 -03:32:34.1 -- not an asteroid (will add it to exclusion list)
07:13:31.49 -03:31:15.0 -- not an asteroid (will add it to exclusion list)
07:15:56.84 -02:38:27.4 -- not an asteroid (will add it to exclusion list)
07:09:03.94 -01:19:31.7 -- not an asteroid (will add it to exclusion list)
06:41:44.27 +00:27:32.2 -- not an asteroid (will add it to exclusion list)
07:08:21.67 -02:47:08.8 -- not an asteroid (will add it to exclusion list)
06:54:54.86 -05:37:07.2 -- not an asteroid (will add it to exclusion list)
06:40:43.75 -01:24:08.9 -- not an asteroid (will add it to exclusion list)
07:03:25.18 -05:00:40.9 -- not an asteroid (will add it to exclusion list)
07:07:24.48 +02:31:26.3 -- not an asteroid (will add it to exclusion list)
07:10:33.35 -03:53:37.9 -- not an asteroid (will add it to exclusion list)
06:48:07.73 -00:40:39.4 -- not an asteroid (will add it to exclusion list)
07:09:53.16 -04:01:41.0 -- not an asteroid (will add it to exclusion list)
06:49:26.81 +02:25:17.1 -- not an asteroid (will add it to exclusion list)
07:09:41.50 -00:55:18.0 -- not an asteroid (will add it to exclusion list)
07:11:44.10 -02:16:15.2 -- not an asteroid (will add it to exclusion list)
06:20:52.80 -06:29:09.0 -- not an asteroid (will add it to exclusion list)
07:09:57.99 +00:39:43.3 -- not an asteroid (will add it to exclusion list)
07:06:38.15 -03:18:51.8 -- not an asteroid (will add it to exclusion list)
06:49:46.90 -00:33:11.0 -- not an asteroid (will add it to exclusion list)
07:06:31.58 +02:11:38.1 -- not an asteroid (will add it to exclusion list)
06:51:28.89 +01:57:04.1 -- not an asteroid (will add it to exclusion list)
06:46:51.22 +02:33:26.9 -- not an asteroid (will add it to exclusion list)
06:35:07.51 -03:03:03.7 -- not an asteroid (will add it to exclusion list)
06:51:38.75 +00:29:29.5 -- not an asteroid (will add it to exclusion list)
06:59:30.47 +00:22:09.3 -- not an asteroid (will add it to exclusion list)
06:58:50.06 -01:53:08.6 -- not an asteroid (will add it to exclusion list)
06:43:52.85 +01:17:52.3 -- not an asteroid (will add it to exclusion list)
07:10:56.75 -04:18:47.4 -- not an asteroid (will add it to exclusion list)
06:59:00.55 -01:39:58.3 -- not an asteroid (will add it to exclusion list)
06:58:57.14 -03:00:40.9 -- not an asteroid (will add it to exclusion list)
07:05:50.92 -02:05:11.4 -- not an asteroid (will add it to exclusion list)
06:44:31.32 -01:39:34.8 -- not an asteroid (will add it to exclusion list)
07:10:41.28 -05:05:03.5 -- not an asteroid (will add it to exclusion list)
07:18:05.05 -01:25:37.6 -- not an asteroid (will add it to exclusion list)
07:18:41.82 +01:11:02.2 -- not an asteroid (will add it to exclusion list)
06:59:36.64 +00:07:21.1 -- not an asteroid (will add it to exclusion list)
06:40:55.32 +00:01:28.0 -- not an asteroid (will add it to exclusion list)
07:04:15.82 -02:22:56.6 -- not an asteroid (will add it to exclusion list)
07:03:52.92 +00:49:49.7 -- not an asteroid (will add it to exclusion list)
06:43:27.90 -03:56:28.1 -- not an asteroid (will add it to exclusion list)
06:54:34.47 -00:35:22.0 -- not an asteroid (will add it to exclusion list)
07:07:26.03 -02:04:10.9 -- not an asteroid (will add it to exclusion list)
07:16:13.34 -00:00:45.0 -- not an asteroid (will add it to exclusion list)
07:06:44.65 -01:25:53.6 -- not an asteroid (will add it to exclusion list)
06:50:09.06 +00:56:41.7 -- not an asteroid (will add it to exclusion list)
06:27:59.03 +02:56:17.9 -- not an asteroid (will add it to exclusion list)
06:53:11.77 -01:33:37.4 -- not an asteroid (will add it to exclusion list)
07:17:50.85 -01:41:23.2 -- not an asteroid (will add it to exclusion list)
06:38:27.90 +00:48:37.4 -- not an asteroid (will add it to exclusion list)
06:48:15.59 +01:46:16.7 -- not an asteroid (will add it to exclusion list)
07:08:35.63 +01:46:44.5 -- not an asteroid (will add it to exclusion list)
06:44:27.39 +02:30:56.5 -- not an asteroid (will add it to exclusion list)
06:40:30.51 -01:04:41.8 -- not an asteroid (will add it to exclusion list)
07:00:03.22 -03:18:50.4 -- not an asteroid (will add it to exclusion list)
07:04:20.46 -02:13:19.9 -- not an asteroid (will add it to exclusion list)
07:09:20.66 +02:38:45.4 -- not an asteroid (will add it to exclusion list)
07:17:52.78 +00:17:04.5 -- not an asteroid (will add it to exclusion list)
07:14:00.02 -02:51:46.6 -- not an asteroid (will add it to exclusion list)
06:57:16.43 -00:59:39.7 -- not an asteroid (will add it to exclusion list)
07:05:12.10 -03:19:35.2 -- not an asteroid (will add it to exclusion list)
07:13:04.82 -05:12:23.7 -- not an asteroid (will add it to exclusion list)
06:56:02.88 +02:23:22.8 -- not an asteroid (will add it to exclusion list)
07:09:32.63 -07:02:49.6 -- not an asteroid (will add it to exclusion list)
06:58:25.52 -02:40:32.3 -- not an asteroid (will add it to exclusion list)
07:18:20.90 -04:33:02.4 -- not an asteroid (will add it to exclusion list)
07:09:56.52 -04:34:52.0 -- not an asteroid (will add it to exclusion list)
06:44:07.44 +03:13:07.3 -- not an asteroid (will add it to exclusion list)
07:20:03.74 -01:48:50.7 -- not an asteroid (will add it to exclusion list)
07:04:34.96 -05:56:29.3 -- not an asteroid (will add it to exclusion list)
07:07:47.05 -02:49:20.6 -- not an asteroid (will add it to exclusion list)
07:13:59.20 -01:53:59.9 -- not an asteroid (will add it to exclusion list)
07:18:29.90 -00:11:36.0 -- not an asteroid (will add it to exclusion list)
07:03:52.72 -06:00:22.1 -- not an asteroid (will add it to exclusion list)
07:18:50.17 -05:15:14.2 -- not an asteroid (will add it to exclusion list)
07:22:02.45 +00:44:40.0 -- not an asteroid (will add it to exclusion list)
07:00:50.76 -00:35:32.2 -- not an asteroid (will add it to exclusion list)
07:10:37.59 -04:15:17.2 -- not an asteroid (will add it to exclusion list)
06:58:59.43 -04:37:56.0 -- not an asteroid (will add it to exclusion list)
07:09:05.02 -02:57:17.9 -- not an asteroid (will add it to exclusion list)
06:45:57.94 +02:35:25.9 -- not an asteroid (will add it to exclusion list)
07:05:14.45 +00:02:10.5 -- not an asteroid (will add it to exclusion list)
07:20:50.53 -00:51:20.8 -- not an asteroid (will add it to exclusion list)
07:10:06.16 +01:43:43.3 -- not an asteroid (will add it to exclusion list)
07:03:04.48 -01:18:36.8 -- not an asteroid (will add it to exclusion list)
07:04:46.61 +02:30:42.1 -- not an asteroid (will add it to exclusion list)
07:10:18.75 -01:17:09.9 -- not an asteroid (will add it to exclusion list)
07:04:16.87 -03:01:37.5 -- not an asteroid (will add it to exclusion list)
07:18:13.69 -00:07:39.7 -- not an asteroid (will add it to exclusion list)
06:42:33.23 -03:28:05.7 -- not an asteroid (will add it to exclusion list)
06:44:36.29 +01:45:28.2 -- not an asteroid (will add it to exclusion list)
07:04:50.40 -01:48:49.9 -- not an asteroid (will add it to exclusion list)
07:15:26.05 -01:11:22.1 -- not an asteroid (will add it to exclusion list)
07:18:48.74 -01:43:48.1 -- not an asteroid (will add it to exclusion list)
07:00:33.81 +02:26:36.6 -- not an asteroid (will add it to exclusion list)
07:05:47.20 +00:13:23.9 -- not an asteroid (will add it to exclusion list)
07:06:45.74 -01:30:47.8 -- not an asteroid (will add it to exclusion list)
06:44:16.60 -00:10:04.5 -- not an asteroid (will add it to exclusion list)
07:06:45.92 -02:11:02.4 -- not an asteroid (will add it to exclusion list)
07:04:10.15 -05:04:53.2 -- not an asteroid (will add it to exclusion list)
07:03:36.84 +02:37:09.8 -- not an asteroid (will add it to exclusion list)
07:01:14.54 +00:57:28.0 -- not an asteroid (will add it to exclusion list)
07:07:33.33 -03:25:29.3 -- not an asteroid (will add it to exclusion list)
06:58:50.18 -04:41:10.7 -- not an asteroid (will add it to exclusion list)
06:57:12.52 -03:57:43.6 -- not an asteroid (will add it to exclusion list)
06:30:03.32 +01:18:34.6 -- not an asteroid (will add it to exclusion list)
06:43:42.42 -04:26:30.3 -- not an asteroid (will add it to exclusion list)
07:08:04.57 -01:43:40.4 -- not an asteroid (will add it to exclusion list)
06:35:48.00 +00:35:27.1 -- not an asteroid (will add it to exclusion list)
07:09:28.93 -06:44:36.9 -- not an asteroid (will add it to exclusion list)
07:00:38.69 -01:30:47.6 -- not an asteroid (will add it to exclusion list)
07:02:49.55 -03:11:38.7 -- not an asteroid (will add it to exclusion list)
06:52:47.86 -06:19:16.6 -- not an asteroid (will add it to exclusion list)
07:03:07.07 +01:49:30.2 -- not an asteroid (will add it to exclusion list)
07:06:46.71 -01:31:18.8 -- not an asteroid (will add it to exclusion list)
07:08:46.29 -02:21:32.3 -- not an asteroid (will add it to exclusion list)
06:54:39.52 +02:38:02.4 -- not an asteroid (will add it to exclusion list)
07:14:23.44 -03:02:00.2 -- not an asteroid (will add it to exclusion list)
07:17:28.58 -01:37:03.7 -- not an asteroid (will add it to exclusion list)
06:46:51.11 +01:18:12.2 -- not an asteroid (will add it to exclusion list)
06:43:55.65 -05:03:59.7 -- not an asteroid (will add it to exclusion list)
07:05:31.89 +02:04:00.7 -- not an asteroid (will add it to exclusion list)
07:09:14.75 -04:55:03.5 -- not an asteroid (will add it to exclusion list)
07:08:52.68 -03:55:18.7 -- not an asteroid (will add it to exclusion list)
06:30:50.32 +02:31:12.6 -- not an asteroid (will add it to exclusion list)
06:39:05.86 +02:23:36.1 -- not an asteroid (will add it to exclusion list)
06:26:38.99 +00:26:39.6 -- not an asteroid (will add it to exclusion list)
06:51:18.33 -01:23:06.9 -- not an asteroid (will add it to exclusion list)
07:10:24.71 +02:20:19.3 -- not an asteroid (will add it to exclusion list)
07:03:51.49 -02:54:47.5 -- not an asteroid (will add it to exclusion list)
06:24:33.54 -01:26:12.8 -- not an asteroid (will add it to exclusion list)
07:13:48.38 +02:30:37.2 -- not an asteroid (will add it to exclusion list)
06:44:48.93 +01:46:41.7 -- not an asteroid (will add it to exclusion list)
07:07:40.35 -03:15:03.6 -- not an asteroid (will add it to exclusion list)
07:05:35.93 -05:43:55.7 -- not an asteroid (will add it to exclusion list)
07:01:15.44 -00:32:58.1 -- not an asteroid (will add it to exclusion list)
07:06:54.26 +02:10:49.8 -- not an asteroid (will add it to exclusion list)
07:21:49.99 +00:09:23.1 -- not an asteroid (will add it to exclusion list)
07:03:46.87 -01:04:50.3 -- not an asteroid (will add it to exclusion list)
06:42:30.97 -06:04:20.5 -- not an asteroid (will add it to exclusion list)
07:12:41.75 -00:50:01.0 -- not an asteroid (will add it to exclusion list)
06:57:35.67 +01:13:53.9 -- not an asteroid (will add it to exclusion list)
07:04:51.68 -02:12:03.7 -- not an asteroid (will add it to exclusion list)
07:19:27.26 -01:40:46.3 -- not an asteroid (will add it to exclusion list)
06:45:17.61 +00:43:40.6 -- not an asteroid (will add it to exclusion list)
06:44:50.83 +01:05:45.3 -- not an asteroid (will add it to exclusion list)
06:53:02.93 +01:17:29.4 -- not an asteroid (will add it to exclusion list)
07:05:38.60 +01:26:03.3 -- not an asteroid (will add it to exclusion list)
06:59:44.43 -01:15:43.0 -- not an asteroid (will add it to exclusion list)
07:15:43.74 -05:23:23.8 -- not an asteroid (will add it to exclusion list)
07:10:24.17 -06:40:08.5 -- not an asteroid (will add it to exclusion list)
07:20:57.72 -02:33:20.3 -- not an asteroid (will add it to exclusion list)
07:18:39.14 -01:16:48.8 -- not an asteroid (will add it to exclusion list)
07:04:10.46 -04:42:09.2 -- not an asteroid (will add it to exclusion list)
07:08:58.19 -02:02:48.7 -- not an asteroid (will add it to exclusion list)
07:08:43.25 +01:18:05.6 -- not an asteroid (will add it to exclusion list)
06:45:39.12 +02:45:26.4 -- not an asteroid (will add it to exclusion list)
07:18:36.19 -02:04:59.2 -- not an asteroid (will add it to exclusion list)
06:58:22.45 -02:33:50.6 -- not an asteroid (will add it to exclusion list)
06:49:45.68 +00:30:49.8 -- not an asteroid (will add it to exclusion list)
06:40:57.09 -04:34:47.9 -- not an asteroid (will add it to exclusion list)
06:41:21.21 -01:43:16.1 -- not an asteroid (will add it to exclusion list)
07:07:24.10 -01:20:23.6 -- not an asteroid (will add it to exclusion list)
07:12:56.48 -03:02:53.3 -- not an asteroid (will add it to exclusion list)
06:54:26.63 +02:55:34.7 -- not an asteroid (will add it to exclusion list)
06:37:05.74 +03:07:56.0 -- not an asteroid (will add it to exclusion list)
07:10:10.81 -02:02:45.9 -- not an asteroid (will add it to exclusion list)
06:55:19.16 +03:02:04.9 -- not an asteroid (will add it to exclusion list)
06:58:38.46 -00:18:50.6 -- not an asteroid (will add it to exclusion list)
06:47:23.79 +01:25:44.9 -- not an asteroid (will add it to exclusion list)
07:09:31.15 -03:28:26.8 -- not an asteroid (will add it to exclusion list)
06:46:57.58 -02:12:24.5 -- not an asteroid (will add it to exclusion list)
07:09:54.20 -04:46:45.0 -- not an asteroid (will add it to exclusion list)
07:09:21.65 +01:07:27.7 -- not an asteroid (will add it to exclusion list)
07:20:15.64 -06:40:49.0 -- not an asteroid (will add it to exclusion list)
06:47:26.83 -04:24:09.2 -- not an asteroid (will add it to exclusion list)
06:47:12.01 +00:21:20.6 -- not an asteroid (will add it to exclusion list)
06:58:48.13 -00:36:46.3 -- not an asteroid (will add it to exclusion list)
06:57:27.64 -05:05:42.1 -- not an asteroid (will add it to exclusion list)
07:16:37.63 -05:50:18.1 -- not an asteroid (will add it to exclusion list)
06:59:02.02 +00:56:30.5 -- not an asteroid (will add it to exclusion list)
07:20:44.76 -05:00:17.0 -- not an asteroid (will add it to exclusion list)
06:51:36.62 -02:04:10.3 -- not an asteroid (will add it to exclusion list)
07:09:46.21 -00:21:13.3 -- not an asteroid (will add it to exclusion list)
06:52:56.87 -04:25:00.4 -- not an asteroid (will add it to exclusion list)
07:19:50.28 -02:33:24.7 -- not an asteroid (will add it to exclusion list)
06:53:52.28 -02:12:22.5 -- not an asteroid (will add it to exclusion list)
06:47:32.89 -01:03:01.2 -- not an asteroid (will add it to exclusion list)
07:12:26.26 -04:38:59.7 -- not an asteroid (will add it to exclusion list)
07:11:11.54 -00:11:45.1 -- not an asteroid (will add it to exclusion list)
06:48:23.32 -05:30:22.9 -- not an asteroid (will add it to exclusion list)
07:02:37.86 -01:54:03.1 -- not an asteroid (will add it to exclusion list)
06:50:41.50 -00:31:44.2 -- not an asteroid (will add it to exclusion list)
06:38:47.12 +02:03:09.6 -- not an asteroid (will add it to exclusion list)
07:00:20.78 -02:22:07.1 -- not an asteroid (will add it to exclusion list)
07:08:10.79 -03:12:34.2 -- not an asteroid (will add it to exclusion list)
07:06:37.06 -01:28:47.0 -- not an asteroid (will add it to exclusion list)
06:43:53.90 +01:01:54.9 -- not an asteroid (will add it to exclusion list)
06:38:18.59 -03:21:22.6 -- not an asteroid (will add it to exclusion list)
06:59:00.99 -02:36:02.6 -- not an asteroid (will add it to exclusion list)
07:02:55.72 -02:02:36.8 -- not an asteroid (will add it to exclusion list)
06:48:12.15 -00:18:59.5 -- not an asteroid (will add it to exclusion list)
06:31:58.75 -03:49:54.8 -- not an asteroid (will add it to exclusion list)
06:41:21.16 -00:35:21.7 -- not an asteroid (will add it to exclusion list)
07:05:47.79 +00:29:04.8 -- not an asteroid (will add it to exclusion list)
06:46:18.44 -02:26:01.1 -- not an asteroid (will add it to exclusion list)
06:51:28.43 -00:06:28.0 -- not an asteroid (will add it to exclusion list)
07:08:47.42 -00:37:49.3 -- not an asteroid (will add it to exclusion list)
07:04:40.36 -01:02:13.7 -- not an asteroid (will add it to exclusion list)
06:38:32.13 +02:21:50.6 -- not an asteroid (will add it to exclusion list)
06:56:37.89 +00:11:26.0 -- not an asteroid (will add it to exclusion list)
06:32:57.59 -02:23:11.8 -- not an asteroid (will add it to exclusion list)
07:14:42.78 -02:55:32.3 -- not an asteroid (will add it to exclusion list)
07:05:05.62 +02:17:06.7 -- not an asteroid (will add it to exclusion list)
06:55:34.59 +01:52:30.2 -- not an asteroid (will add it to exclusion list)
06:47:10.53 +02:54:04.4 -- not an asteroid (will add it to exclusion list)
07:21:37.13 +02:27:48.5 -- not an asteroid (will add it to exclusion list)
07:11:24.98 -05:58:01.4 -- not an asteroid (will add it to exclusion list)
06:45:54.15 -00:09:36.4 -- not an asteroid (will add it to exclusion list)
06:54:01.69 -02:07:17.0 -- not an asteroid (will add it to exclusion list)
07:07:15.74 +02:06:37.0 -- not an asteroid (will add it to exclusion list)
06:38:15.57 +00:43:52.6 -- not an asteroid (will add it to exclusion list)
06:51:24.01 +00:52:45.8 -- not an asteroid (will add it to exclusion list)
06:56:41.81 -00:14:41.1 -- not an asteroid (will add it to exclusion list)
06:53:39.64 +00:03:18.3 -- not an asteroid (will add it to exclusion list)
07:00:12.27 -01:50:10.3 -- not an asteroid (will add it to exclusion list)
07:12:49.07 -03:33:13.0 -- not an asteroid (will add it to exclusion list)
06:58:34.56 -01:38:22.8 -- not an asteroid (will add it to exclusion list)
06:55:50.76 -02:12:27.4 -- not an asteroid (will add it to exclusion list)
06:38:37.28 -02:20:02.8 -- not an asteroid (will add it to exclusion list)
06:56:31.80 +02:40:02.5 -- not an asteroid (will add it to exclusion list)
07:11:22.90 -03:40:07.3 -- not an asteroid (will add it to exclusion list)
06:57:32.77 -05:57:35.7 -- not an asteroid (will add it to exclusion list)
06:40:47.22 -01:31:42.0 -- not an asteroid (will add it to exclusion list)
06:44:36.38 -00:34:40.8 -- not an asteroid (will add it to exclusion list)
07:13:09.03 +02:42:09.3 -- not an asteroid (will add it to exclusion list)
06:59:18.34 +02:00:31.3 -- not an asteroid (will add it to exclusion list)
06:51:11.58 -02:22:08.9 -- not an asteroid (will add it to exclusion list)
07:07:29.49 +01:15:34.1 -- not an asteroid (will add it to exclusion list)
07:21:08.26 -01:43:14.9 -- not an asteroid (will add it to exclusion list)
06:20:28.15 -03:16:34.6 -- not an asteroid (will add it to exclusion list)
06:55:46.11 +00:37:44.4 -- not an asteroid (will add it to exclusion list)
07:11:46.28 +01:10:54.4 -- not an asteroid (will add it to exclusion list)
07:09:19.51 -00:22:15.1 -- not an asteroid (will add it to exclusion list)
07:09:25.87 -02:13:07.3 -- not an asteroid (will add it to exclusion list)
06:58:11.17 -02:26:27.3 -- not an asteroid (will add it to exclusion list)
06:50:55.39 -01:20:54.8 -- not an asteroid (will add it to exclusion list)
06:52:15.51 -01:19:38.7 -- not an asteroid (will add it to exclusion list)
07:00:32.43 -03:26:18.3 -- not an asteroid (will add it to exclusion list)
07:09:37.91 -00:01:16.9 -- not an asteroid (will add it to exclusion list)
07:01:45.48 -00:36:23.3 -- not an asteroid (will add it to exclusion list)
07:19:23.84 +00:34:10.6 -- not an asteroid (will add it to exclusion list)
06:48:04.27 -01:54:51.4 -- not an asteroid (will add it to exclusion list)
07:07:16.70 +01:31:11.8 -- not an asteroid (will add it to exclusion list)
07:04:19.83 +00:50:07.3 -- not an asteroid (will add it to exclusion list)
06:56:25.52 -03:54:41.1 -- not an asteroid (will add it to exclusion list)
07:05:44.24 -02:20:49.5 -- not an asteroid (will add it to exclusion list)
06:24:14.93 +00:04:42.4 -- not an asteroid (will add it to exclusion list)
06:26:19.97 -00:45:06.8 -- not an asteroid (will add it to exclusion list)
07:03:50.85 -01:11:02.4 -- not an asteroid (will add it to exclusion list)
06:55:03.30 +01:21:34.7 -- not an asteroid (will add it to exclusion list)
06:42:39.85 +01:17:02.6 -- not an asteroid (will add it to exclusion list)
06:56:06.42 -04:22:09.2 -- not an asteroid (will add it to exclusion list)
07:05:41.38 -03:03:49.3 -- not an asteroid (will add it to exclusion list)
06:45:15.40 -00:22:56.5 -- not an asteroid (will add it to exclusion list)
07:20:06.00 -02:24:28.4 -- not an asteroid (will add it to exclusion list)
07:03:44.53 -02:34:43.9 -- not an asteroid (will add it to exclusion list)
06:46:37.95 +02:08:17.8 -- not an asteroid (will add it to exclusion list)
06:30:03.84 -01:08:31.7 -- not an asteroid (will add it to exclusion list)
06:57:58.69 -05:42:47.1 -- not an asteroid (will add it to exclusion list)
07:10:48.74 -05:12:39.3 -- not an asteroid (will add it to exclusion list)
07:07:21.15 +00:33:34.9 -- not an asteroid (will add it to exclusion list)
06:51:46.23 +02:39:47.7 -- not an asteroid (will add it to exclusion list)
07:07:11.77 -02:35:01.6 -- not an asteroid (will add it to exclusion list)
07:12:42.54 -04:10:12.5 -- not an asteroid (will add it to exclusion list)
07:19:12.60 -01:22:35.5 -- not an asteroid (will add it to exclusion list)
07:01:15.43 -05:20:34.3 -- not an asteroid (will add it to exclusion list)
07:18:32.61 -01:20:52.4 -- not an asteroid (will add it to exclusion list)
07:18:52.05 -03:35:10.6 -- not an asteroid (will add it to exclusion list)
07:09:40.33 -02:29:08.6 -- not an asteroid (will add it to exclusion list)
06:46:04.24 -02:35:17.2 -- not an asteroid (will add it to exclusion list)
07:01:56.05 +01:13:08.5 -- not an asteroid (will add it to exclusion list)
06:54:09.36 +01:41:25.2 -- not an asteroid (will add it to exclusion list)
06:41:04.21 +02:37:12.2 -- not an asteroid (will add it to exclusion list)
07:12:49.59 -00:29:11.3 -- not an asteroid (will add it to exclusion list)
06:55:56.32 +02:39:57.1 -- not an asteroid (will add it to exclusion list)
07:19:52.56 +00:18:03.9 -- not an asteroid (will add it to exclusion list)
06:48:44.11 +02:30:00.2 -- not an asteroid (will add it to exclusion list)
07:03:53.59 +01:24:55.8 -- not an asteroid (will add it to exclusion list)
07:19:04.11 +00:51:17.9 -- not an asteroid (will add it to exclusion list)
07:12:45.14 +01:18:47.2 -- not an asteroid (will add it to exclusion list)
07:01:12.84 -03:51:27.8 -- not an asteroid (will add it to exclusion list)
06:57:20.23 -01:46:09.4 -- not an asteroid (will add it to exclusion list)
07:03:48.73 -01:24:40.5 -- not an asteroid (will add it to exclusion list)
06:39:06.21 +00:32:11.4 -- not an asteroid (will add it to exclusion list)
07:12:23.96 -02:24:26.6 -- not an asteroid (will add it to exclusion list)
07:10:31.33 -00:55:56.3 -- not an asteroid (will add it to exclusion list)
07:02:28.55 +02:29:05.2 -- not an asteroid (will add it to exclusion list)
07:06:40.26 +00:42:28.4 -- not an asteroid (will add it to exclusion list)
06:54:13.65 +02:59:21.4 -- not an asteroid (will add it to exclusion list)
06:36:38.11 -00:15:14.8 -- not an asteroid (will add it to exclusion list)
06:52:19.06 +00:50:21.6 -- not an asteroid (will add it to exclusion list)
06:56:18.54 -02:55:33.0 -- not an asteroid (will add it to exclusion list)
07:12:18.57 -03:48:49.1 -- not an asteroid (will add it to exclusion list)
06:57:56.59 -02:44:53.0 -- not an asteroid (will add it to exclusion list)
06:57:19.64 -02:37:56.7 -- not an asteroid (will add it to exclusion list)
06:54:40.17 -00:46:47.9 -- not an asteroid (will add it to exclusion list)
07:01:14.59 +01:01:15.8 -- not an asteroid (will add it to exclusion list)
06:53:03.14 -00:27:34.5 -- not an asteroid (will add it to exclusion list)
06:45:14.28 -01:50:55.9 -- not an asteroid (will add it to exclusion list)
07:17:27.14 -00:59:54.5 -- not an asteroid (will add it to exclusion list)
07:02:55.58 +02:43:40.0 -- not an asteroid (will add it to exclusion list)
06:59:50.28 -01:50:11.7 -- not an asteroid (will add it to exclusion list)
07:00:23.20 +00:26:32.7 -- not an asteroid (will add it to exclusion list)
06:48:40.33 -01:40:12.9 -- not an asteroid (will add it to exclusion list)
06:30:11.45 +01:52:29.9 -- not an asteroid (will add it to exclusion list)
07:22:26.05 +00:56:45.9 -- not an asteroid (will add it to exclusion list)
07:19:10.41 -01:27:06.6 -- not an asteroid (will add it to exclusion list)
07:02:53.40 -01:36:00.2 -- not an asteroid (will add it to exclusion list)
07:08:53.87 +00:51:37.1 -- not an asteroid (will add it to exclusion list)
06:52:30.57 -02:40:20.2 -- not an asteroid (will add it to exclusion list)
06:59:26.22 -00:40:38.3 -- not an asteroid (will add it to exclusion list)
07:09:39.99 +01:41:30.4 -- not an asteroid (will add it to exclusion list)
06:45:28.49 +01:05:23.4 -- not an asteroid (will add it to exclusion list)
06:47:34.69 +02:44:50.8 -- not an asteroid (will add it to exclusion list)
06:45:45.32 +01:55:47.1 -- not an asteroid (will add it to exclusion list)
07:09:13.72 -02:21:30.7 -- not an asteroid (will add it to exclusion list)
07:08:45.34 +00:41:48.8 -- not an asteroid (will add it to exclusion list)
07:17:31.25 +01:05:39.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:20:28.15 -03:16:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:52.80 -06:29:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:14.93 +00:04:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:33.54 -01:26:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.97 -00:45:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:38.99 +00:26:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:15.29 +03:07:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:59.03 +02:56:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:54.41 +03:09:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:03.32 +01:18:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:03.84 -01:08:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:11.45 +01:52:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:15.33 +02:16:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:50.32 +02:31:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:58.75 -03:49:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:57.59 -02:23:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:07.51 -03:03:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:48.00 +00:35:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:38.11 -00:15:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:05.74 +03:07:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:31.98 +01:46:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:53.00 -05:55:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:15.57 +00:43:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:18.59 -03:21:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:27.90 +00:48:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:28.20 +00:44:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:32.13 +02:21:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:37.28 -02:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:47.12 +02:03:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:05.86 +02:23:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:06.21 +00:32:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.51 -01:04:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:43.75 -01:24:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:47.22 -01:31:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:55.32 +00:01:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:57.09 -04:34:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:01.89 -01:17:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:04.21 +02:37:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.16 -00:35:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.21 -01:43:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.78 +02:48:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:43.15 +02:53:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:44.27 +00:27:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.97 -06:04:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.23 -03:28:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:39.85 +01:17:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.62 +01:58:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:22.52 +01:54:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:27.90 -03:56:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:32.78 +01:24:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:42.42 -04:26:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.63 -05:42:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:52.85 +01:17:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:53.90 +01:01:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:55.65 -05:03:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:07.44 +03:13:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:12.29 -01:09:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:16.02 -03:32:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:16.60 -00:10:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:19.75 -00:03:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:27.39 +02:30:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.32 -01:39:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.29 +01:45:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:36.38 -00:34:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:48.93 +01:46:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.83 +01:05:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:14.28 -01:50:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:15.40 -00:22:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.61 +00:43:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:28.49 +01:05:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:39.12 +02:45:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:45.32 +01:55:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.15 -00:09:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:57.94 +02:35:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:59.75 +01:38:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:04.24 -02:35:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.50 +01:00:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:18.44 -02:26:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:20.89 +02:44:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.69 -00:28:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:26.75 +00:59:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.35 +01:08:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:37.95 +02:08:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:38.75 +00:42:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:51.11 +01:18:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:51.22 +02:33:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:56.80 +01:41:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:57.58 -02:12:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.53 +02:54:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:12.01 +00:21:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:23.79 +01:25:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:26.83 -04:24:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:32.89 -01:03:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:34.69 +02:44:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:37.26 +01:42:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:04.27 -01:54:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:07.73 -00:40:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:12.15 -00:18:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.59 +01:46:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:23.32 -05:30:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:33.32 +01:48:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:40.33 -01:40:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:44.11 +02:30:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:26.81 +02:25:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:31.01 +01:58:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:45.68 +00:30:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:46.90 -00:33:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.06 +00:56:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:11.49 +02:16:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.50 -00:31:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:55.39 -01:20:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:11.58 -02:22:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.33 -01:23:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.80 +02:12:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:22.46 +00:33:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:24.01 +00:52:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.43 -00:06:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.89 +01:57:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:36.62 -02:04:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:38.75 +00:29:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:46.23 +02:39:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:53.52 +02:07:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:15.51 -01:19:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:19.06 +00:50:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:30.57 -02:40:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:47.86 -06:19:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:56.87 -04:25:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:02.93 +01:17:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:03.14 -00:27:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:11.77 -01:33:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:18.48 +01:05:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:34.07 -00:32:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:35.64 -01:35:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:39.64 +00:03:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.61 -01:58:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.01 +01:14:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:51.74 -01:16:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.28 -02:12:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:01.69 -02:07:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:06.97 -01:31:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:09.36 +01:41:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:13.65 +02:59:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:26.63 +02:55:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.47 -00:35:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.63 -00:15:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.03 +00:12:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.52 +02:38:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.98 +01:28:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:40.17 -00:46:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:46.97 -00:18:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:54.86 -05:37:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:03.30 +01:21:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:07.90 -00:16:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:19.16 +03:02:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:34.59 +01:52:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:40.68 -00:18:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:46.11 +00:37:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.76 -02:12:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:56.32 +02:39:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:57.57 +02:33:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:02.88 +02:23:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:04.66 -01:29:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:06.42 -04:22:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:17.04 +00:50:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:18.54 -02:55:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:25.52 -03:54:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:31.80 +02:40:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:37.89 +00:11:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:41.81 -00:14:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:43.24 -02:17:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:45.76 -01:04:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.52 -03:57:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.43 -00:59:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:19.64 -02:37:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:20.23 -01:46:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.64 -05:05:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:32.77 -05:57:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.67 +01:13:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:56.59 -02:44:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:58.69 -05:42:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:00.79 -01:28:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:11.17 -02:26:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.45 -02:33:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:25.52 -02:40:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.56 -01:38:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:38.46 -00:18:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:48.13 -00:36:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.06 -01:53:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.18 -04:41:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:51.94 +02:39:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.14 -03:00:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:59.43 -04:37:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.55 -01:39:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.99 -02:36:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:02.02 +00:56:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:07.03 +00:37:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:18.34 +02:00:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:26.22 -00:40:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.47 +00:22:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:36.64 +00:07:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:44.43 -01:15:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:50.28 -01:50:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:03.22 -03:18:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:12.27 -01:50:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:20.78 -02:22:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:23.20 +00:26:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:32.06 +01:06:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:32.43 -03:26:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:33.81 +02:26:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:38.69 -01:30:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:46.29 +02:09:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:50.76 -00:35:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:58.00 -02:15:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:04.17 -04:48:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:12.84 -03:51:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.54 +00:57:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.59 +01:01:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.43 -05:20:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.44 -00:32:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.91 +02:06:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:18.85 -01:50:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:34.28 -00:13:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:45.48 -00:36:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:50.23 -01:29:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:53.81 +01:22:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:56.05 +01:13:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:01.21 +00:39:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.51 -01:34:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:28.55 +02:29:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.38 -00:13:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:37.86 -01:54:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:49.55 -03:11:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:52.15 +00:55:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:53.40 -01:36:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:55.58 +02:43:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:55.72 -02:02:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.48 -01:18:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:07.07 +01:49:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.18 -05:00:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.84 +02:37:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:37.02 -00:12:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:39.79 -04:38:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:44.53 -02:34:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:46.87 -01:04:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:48.73 -01:24:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:50.85 -01:11:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:51.49 -02:54:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.72 -06:00:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.92 +00:49:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:53.59 +01:24:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.15 -05:04:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.46 -04:42:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:15.82 -02:22:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.87 -03:01:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:18.10 -00:12:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:19.83 +00:50:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.04 +02:37:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:20.46 -02:13:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:22.70 +00:59:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:34.81 -03:53:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:34.96 -05:56:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:40.36 -01:02:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:46.61 +02:30:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:50.40 -01:48:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.68 -02:12:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.62 +02:17:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:12.10 -03:19:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.45 +00:02:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:15.99 -05:50:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.12 -02:51:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:24.62 -01:37:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:31.89 +02:04:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:35.93 -05:43:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.60 +01:26:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:41.38 -03:03:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:44.24 -02:20:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.73 -02:32:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:47.20 +00:13:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:47.79 +00:29:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.92 -02:05:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:13.57 -05:05:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:26.93 -02:45:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.58 +02:11:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.74 +01:08:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:37.06 -01:28:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:38.15 -03:18:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:40.26 +00:42:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:44.65 -01:25:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.74 -01:30:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.92 -02:11:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:46.71 -01:31:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:54.26 +02:10:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:11.77 -02:35:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.74 +02:06:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:16.70 +01:31:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:21.15 +00:33:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.10 -01:20:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.48 +02:31:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:26.03 -02:04:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:29.49 +01:15:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:33.33 -03:25:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:40.35 -03:15:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:47.05 -02:49:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:04.57 -01:43:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:10.79 -03:12:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:21.67 -02:47:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.63 +01:46:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.25 +01:18:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.34 +00:41:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:46.29 -02:21:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:47.42 -00:37:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:52.68 -03:55:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:53.87 +00:51:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:57.78 -03:05:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:58.19 -02:02:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:03.94 -01:19:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:05.02 -02:57:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.72 -02:21:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:14.75 -04:55:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:19.51 -00:22:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.66 +02:38:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.65 +01:07:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:25.19 -03:13:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:25.87 -02:13:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:28.93 -06:44:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:31.15 -03:28:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:32.63 -07:02:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:37.91 -00:01:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:39.99 +01:41:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:40.33 -02:29:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:40.95 -04:22:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:41.50 -00:55:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:46.21 -00:21:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:53.16 -04:01:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:53.98 -00:44:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:54.20 -04:46:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:56.52 -04:34:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:57.99 +00:39:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:06.16 +01:43:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.13 -00:55:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.18 -00:03:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.81 -02:02:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:12.62 +01:37:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:18.75 -01:17:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:24.17 -06:40:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:24.71 +02:20:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:31.33 -00:55:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:32.61 -05:43:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:33.35 -03:53:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:37.59 -04:15:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:41.28 -05:05:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:48.74 -05:12:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:56.75 -04:18:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:11.54 -00:11:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.91 -03:51:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:22.90 -03:40:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:24.98 -05:58:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:44.10 -02:16:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:46.28 +01:10:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:04.38 -02:55:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:17.29 -02:11:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:18.57 -03:48:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:23.96 -02:24:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:26.26 -04:38:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:39.39 -00:37:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:41.75 -00:50:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:42.54 -04:10:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:45.14 +01:18:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.07 -03:33:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.34 -01:30:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:49.59 -00:29:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.48 -03:02:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:04.82 -05:12:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:09.03 +02:42:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:31.49 -03:31:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:32.71 -00:55:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:39.12 -01:41:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:48.38 +02:30:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:59.20 -01:53:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:00.02 -02:51:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:23.44 -03:02:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:42.78 -02:55:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:17.25 -00:21:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:26.05 -01:11:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:27.88 -02:44:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:43.74 -05:23:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:56.84 -02:38:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:08.24 +00:05:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:13.34 -00:00:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:37.63 -05:50:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:13.61 -02:22:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:27.14 -00:59:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:28.58 -01:37:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.25 +01:05:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:36.46 -00:24:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:50.85 -01:41:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:52.78 +00:17:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:05.05 -01:25:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:13.69 -00:07:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:14.13 -05:37:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:20.90 -04:33:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:22.73 +00:37:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:29.90 -00:11:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:32.61 -01:20:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:36.19 -02:04:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:39.14 -01:16:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:41.82 +01:11:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:48.74 -01:43:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:50.17 -05:15:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:52.05 -03:35:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:02.10 -06:31:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:02.35 -07:07:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:04.11 +00:51:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:10.41 -01:27:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:10.42 -01:30:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:12.60 -01:22:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:23.84 +00:34:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:24.04 -02:42:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:26.13 +00:51:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:27.26 -01:40:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:50.28 -02:33:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:52.56 +00:18:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:54.20 -01:00:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:03.74 -01:48:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:06.00 -02:24:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:15.64 -06:40:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:41.08 -03:34:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:43.53 -02:48:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:44.76 -05:00:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:50.53 -00:51:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:57.72 -02:33:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:08.26 -01:43:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:19.45 -02:07:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:21.23 +00:37:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:37.13 +02:27:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:49.99 +00:09:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:02.45 +00:44:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:26.05 +00:56:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:20:28.15 -03:16:34.6 -- not a known variable star
06:20:52.80 -06:29:09.0 -- not a known variable star
06:24:14.93 +00:04:42.4 -- not a known variable star
06:24:33.54 -01:26:12.8 -- a known variable star
06:26:19.97 -00:45:06.8 -- not a known variable star
06:26:38.99 +00:26:39.6 -- not a known variable star
06:27:15.29 +03:07:46.0 -- not a known variable star
06:27:59.03 +02:56:17.9 -- a known variable star
06:29:54.41 +03:09:24.5 -- a known variable star
06:30:03.32 +01:18:34.6 -- a known variable star
06:30:03.84 -01:08:31.7 -- not a known variable star
06:30:11.45 +01:52:29.9 -- not a known variable star
06:30:15.33 +02:16:00.5 -- not a known variable star
06:30:50.32 +02:31:12.6 -- not a known variable star
06:31:58.75 -03:49:54.8 -- not a known variable star
06:32:57.59 -02:23:11.8 -- a known variable star
06:35:07.51 -03:03:03.7 -- not a known variable star
06:35:48.00 +00:35:27.1 -- not a known variable star
06:36:38.11 -00:15:14.8 -- not a known variable star
06:37:05.74 +03:07:56.0 -- not a known variable star
06:37:31.98 +01:46:27.4 -- a known variable star
06:37:53.00 -05:55:11.9 -- a known variable star
06:38:15.57 +00:43:52.6 -- not a known variable star
06:38:18.59 -03:21:22.6 -- not a known variable star
06:38:27.90 +00:48:37.4 -- a known variable star
06:38:28.20 +00:44:36.6 -- a known variable star
06:38:32.13 +02:21:50.6 -- a known variable star
06:38:37.28 -02:20:02.8 -- not a known variable star
06:38:47.12 +02:03:09.6 -- not a known variable star
06:39:05.86 +02:23:36.1 -- a known variable star
06:39:06.21 +00:32:11.4 -- not a known variable star
06:40:30.51 -01:04:41.8 -- a known variable star
06:40:43.75 -01:24:08.9 -- a known variable star
06:40:47.22 -01:31:42.0 -- not a known variable star
06:40:55.32 +00:01:28.0 -- a known variable star
06:40:57.09 -04:34:47.9 -- not a known variable star
06:41:01.89 -01:17:33.8 -- not a known variable star
06:41:04.21 +02:37:12.2 -- not a known variable star
06:41:21.16 -00:35:21.7 -- not a known variable star
06:41:21.21 -01:43:16.1 -- not a known variable star
06:41:26.78 +02:48:00.9 -- not a known variable star
06:41:43.15 +02:53:01.3 -- not a known variable star
06:41:44.27 +00:27:32.2 -- a known variable star
06:42:30.97 -06:04:20.5 -- a known variable star
06:42:33.23 -03:28:05.7 -- not a known variable star
06:42:39.85 +01:17:02.6 -- not a known variable star
06:43:14.62 +01:58:21.4 -- not a known variable star
06:43:22.52 +01:54:52.6 -- not a known variable star
06:43:27.90 -03:56:28.1 -- a known variable star
06:43:32.78 +01:24:34.0 -- not a known variable star
06:43:42.42 -04:26:30.3 -- a known variable star
06:43:46.63 -05:42:06.8 -- not a known variable star
06:43:52.85 +01:17:52.3 -- not a known variable star
06:43:53.90 +01:01:54.9 -- a known variable star
06:43:55.65 -05:03:59.7 -- not a known variable star
06:44:07.44 +03:13:07.3 -- not a known variable star
06:44:12.29 -01:09:13.8 -- a known variable star
06:44:16.02 -03:32:34.1 -- not a known variable star
06:44:16.60 -00:10:04.5 -- not a known variable star
06:44:19.75 -00:03:11.7 -- not a known variable star
06:44:27.39 +02:30:56.5 -- not a known variable star
06:44:31.32 -01:39:34.8 -- not a known variable star
06:44:36.29 +01:45:28.2 -- not a known variable star
06:44:36.38 -00:34:40.8 -- not a known variable star
06:44:48.93 +01:46:41.7 -- not a known variable star
06:44:50.83 +01:05:45.3 -- not a known variable star
06:45:14.28 -01:50:55.9 -- not a known variable star
06:45:15.40 -00:22:56.5 -- not a known variable star
06:45:17.61 +00:43:40.6 -- not a known variable star
06:45:28.49 +01:05:23.4 -- not a known variable star
06:45:39.12 +02:45:26.4 -- a known variable star
06:45:45.32 +01:55:47.1 -- not a known variable star
06:45:54.15 -00:09:36.4 -- not a known variable star
06:45:57.94 +02:35:25.9 -- not a known variable star
06:45:59.75 +01:38:33.5 -- not a known variable star
06:46:04.24 -02:35:17.2 -- not a known variable star
06:46:10.50 +01:00:20.7 -- not a known variable star
06:46:18.44 -02:26:01.1 -- a known variable star
06:46:20.89 +02:44:07.5 -- a known variable star
06:46:25.69 -00:28:35.8 -- not a known variable star
06:46:26.75 +00:59:05.0 -- not a known variable star
06:46:31.35 +01:08:38.5 -- not a known variable star
06:46:37.95 +02:08:17.8 -- not a known variable star
06:46:38.75 +00:42:37.0 -- a known variable star
06:46:51.11 +01:18:12.2 -- a known variable star
06:46:51.22 +02:33:26.9 -- a known variable star
06:46:56.80 +01:41:47.9 -- not a known variable star
06:46:57.58 -02:12:24.5 -- not a known variable star
06:47:10.53 +02:54:04.4 -- not a known variable star
06:47:12.01 +00:21:20.6 -- a known variable star
06:47:23.79 +01:25:44.9 -- not a known variable star
06:47:26.83 -04:24:09.2 -- not a known variable star
06:47:32.89 -01:03:01.2 -- not a known variable star
06:47:34.69 +02:44:50.8 -- a known variable star
06:47:37.26 +01:42:20.5 -- not a known variable star
06:48:04.27 -01:54:51.4 -- not a known variable star
06:48:07.73 -00:40:39.4 -- not a known variable star
06:48:12.15 -00:18:59.5 -- a known variable star
06:48:15.59 +01:46:16.7 -- not a known variable star
06:48:23.32 -05:30:22.9 -- not a known variable star
06:48:33.32 +01:48:57.5 -- a known variable star
06:48:40.33 -01:40:12.9 -- a known variable star
06:48:44.11 +02:30:00.2 -- not a known variable star
06:49:26.81 +02:25:17.1 -- not a known variable star
06:49:31.01 +01:58:03.6 -- not a known variable star
06:49:45.68 +00:30:49.8 -- a known variable star
06:49:46.90 -00:33:11.0 -- not a known variable star
06:50:09.06 +00:56:41.7 -- not a known variable star
06:50:11.49 +02:16:28.9 -- a known variable star
06:50:41.50 -00:31:44.2 -- not a known variable star
06:50:55.39 -01:20:54.8 -- a known variable star
06:51:11.58 -02:22:08.9 -- not a known variable star
06:51:18.33 -01:23:06.9 -- a known variable star
06:51:18.80 +02:12:27.8 -- not a known variable star
06:51:22.46 +00:33:45.3 -- not a known variable star
06:51:24.01 +00:52:45.8 -- not a known variable star
06:51:28.43 -00:06:28.0 -- not a known variable star
06:51:28.89 +01:57:04.1 -- not a known variable star
06:51:36.62 -02:04:10.3 -- a known variable star
06:51:38.75 +00:29:29.5 -- a known variable star
06:51:46.23 +02:39:47.7 -- not a known variable star
06:51:53.52 +02:07:47.6 -- a known variable star
06:52:15.51 -01:19:38.7 -- not a known variable star
06:52:19.06 +00:50:21.6 -- not a known variable star
06:52:30.57 -02:40:20.2 -- not a known variable star
06:52:47.86 -06:19:16.6 -- not a known variable star
06:52:56.87 -04:25:00.4 -- not a known variable star
06:53:02.93 +01:17:29.4 -- a known variable star
06:53:03.14 -00:27:34.5 -- a known variable star
06:53:11.77 -01:33:37.4 -- a known variable star
06:53:18.48 +01:05:30.6 -- a known variable star
06:53:34.07 -00:32:05.1 -- not a known variable star
06:53:35.64 -01:35:01.5 -- a known variable star
06:53:39.64 +00:03:18.3 -- not a known variable star
06:53:43.61 -01:58:40.8 -- not a known variable star
06:53:47.01 +01:14:31.6 -- not a known variable star
06:53:51.74 -01:16:59.6 -- not a known variable star
06:53:52.28 -02:12:22.5 -- not a known variable star
06:54:01.69 -02:07:17.0 -- not a known variable star
06:54:06.97 -01:31:50.2 -- not a known variable star
06:54:09.36 +01:41:25.2 -- not a known variable star
06:54:13.65 +02:59:21.4 -- not a known variable star
06:54:26.63 +02:55:34.7 -- not a known variable star
06:54:34.47 -00:35:22.0 -- not a known variable star
06:54:34.63 -00:15:46.2 -- a known variable star
06:54:39.03 +00:12:16.2 -- a known variable star
06:54:39.52 +02:38:02.4 -- not a known variable star
06:54:39.98 +01:28:18.3 -- a known variable star
06:54:40.17 -00:46:47.9 -- not a known variable star
06:54:46.97 -00:18:59.5 -- a known variable star
06:54:54.86 -05:37:07.2 -- a known variable star
06:55:03.30 +01:21:34.7 -- not a known variable star
06:55:07.90 -00:16:28.5 -- not a known variable star
06:55:19.16 +03:02:04.9 -- not a known variable star
06:55:34.59 +01:52:30.2 -- not a known variable star
06:55:40.68 -00:18:33.0 -- not a known variable star
06:55:46.11 +00:37:44.4 -- not a known variable star
06:55:50.76 -02:12:27.4 -- not a known variable star
06:55:56.32 +02:39:57.1 -- a known variable star
06:55:57.57 +02:33:21.4 -- not a known variable star
06:56:02.88 +02:23:22.8 -- not a known variable star
06:56:04.66 -01:29:54.7 -- not a known variable star
06:56:06.42 -04:22:09.2 -- not a known variable star
06:56:17.04 +00:50:18.8 -- not a known variable star
06:56:18.54 -02:55:33.0 -- not a known variable star
06:56:25.52 -03:54:41.1 -- not a known variable star
06:56:31.80 +02:40:02.5 -- not a known variable star
06:56:37.89 +00:11:26.0 -- not a known variable star
06:56:41.81 -00:14:41.1 -- not a known variable star
06:56:43.24 -02:17:37.5 -- a known variable star
06:56:45.76 -01:04:30.3 -- not a known variable star
06:57:12.52 -03:57:43.6 -- not a known variable star
06:57:16.43 -00:59:39.7 -- not a known variable star
06:57:19.64 -02:37:56.7 -- not a known variable star
06:57:20.23 -01:46:09.4 -- a known variable star
06:57:27.64 -05:05:42.1 -- not a known variable star
06:57:32.77 -05:57:35.7 -- a known variable star
06:57:35.67 +01:13:53.9 -- a known variable star
06:57:56.59 -02:44:53.0 -- not a known variable star
06:57:58.69 -05:42:47.1 -- not a known variable star
06:58:00.79 -01:28:24.0 -- not a known variable star
06:58:11.17 -02:26:27.3 -- not a known variable star
06:58:22.45 -02:33:50.6 -- a known variable star
06:58:25.52 -02:40:32.3 -- a known variable star
06:58:34.56 -01:38:22.8 -- not a known variable star
06:58:38.46 -00:18:50.6 -- not a known variable star
06:58:48.13 -00:36:46.3 -- not a known variable star
06:58:50.06 -01:53:08.6 -- not a known variable star
06:58:50.18 -04:41:10.7 -- not a known variable star
06:58:51.94 +02:39:12.6 -- not a known variable star
06:58:57.14 -03:00:40.9 -- not a known variable star
06:58:59.43 -04:37:56.0 -- not a known variable star
06:59:00.55 -01:39:58.3 -- not a known variable star
06:59:00.99 -02:36:02.6 -- not a known variable star
06:59:02.02 +00:56:30.5 -- not a known variable star
06:59:07.03 +00:37:18.7 -- not a known variable star
06:59:18.34 +02:00:31.3 -- a known variable star
06:59:26.22 -00:40:38.3 -- not a known variable star
06:59:30.47 +00:22:09.3 -- not a known variable star
06:59:36.64 +00:07:21.1 -- not a known variable star
06:59:44.43 -01:15:43.0 -- not a known variable star
06:59:50.28 -01:50:11.7 -- not a known variable star
07:00:03.22 -03:18:50.4 -- not a known variable star
07:00:12.27 -01:50:10.3 -- not a known variable star
07:00:20.78 -02:22:07.1 -- not a known variable star
07:00:23.20 +00:26:32.7 -- not a known variable star
07:00:32.06 +01:06:04.8 -- not a known variable star
07:00:32.43 -03:26:18.3 -- a known variable star
07:00:33.81 +02:26:36.6 -- not a known variable star
07:00:38.69 -01:30:47.6 -- not a known variable star
07:00:46.29 +02:09:09.1 -- not a known variable star
07:00:50.76 -00:35:32.2 -- not a known variable star
07:00:58.00 -02:15:42.6 -- not a known variable star
07:01:04.17 -04:48:05.7 -- a known variable star
07:01:12.84 -03:51:27.8 -- not a known variable star
07:01:14.54 +00:57:28.0 -- not a known variable star
07:01:14.59 +01:01:15.8 -- not a known variable star
07:01:15.43 -05:20:34.3 -- not a known variable star
07:01:15.44 -00:32:58.1 -- a known variable star
07:01:15.91 +02:06:07.1 -- a known variable star
07:01:18.85 -01:50:06.9 -- a known variable star
07:01:34.28 -00:13:23.1 -- not a known variable star
07:01:45.48 -00:36:23.3 -- not a known variable star
07:01:50.23 -01:29:53.3 -- a known variable star
07:01:53.81 +01:22:52.2 -- not a known variable star
07:01:56.05 +01:13:08.5 -- not a known variable star
07:02:01.21 +00:39:08.4 -- not a known variable star
07:02:23.51 -01:34:43.4 -- not a known variable star
07:02:28.55 +02:29:05.2 -- not a known variable star
07:02:32.38 -00:13:08.4 -- not a known variable star
07:02:37.86 -01:54:03.1 -- not a known variable star
07:02:49.55 -03:11:38.7 -- a known variable star
07:02:52.15 +00:55:00.1 -- a known variable star
07:02:53.40 -01:36:00.2 -- not a known variable star
07:02:55.58 +02:43:40.0 -- not a known variable star
07:02:55.72 -02:02:36.8 -- not a known variable star
07:03:04.48 -01:18:36.8 -- not a known variable star
07:03:07.07 +01:49:30.2 -- a known variable star
07:03:25.18 -05:00:40.9 -- a known variable star
07:03:36.84 +02:37:09.8 -- a known variable star
07:03:37.02 -00:12:38.0 -- not a known variable star
07:03:39.79 -04:38:23.8 -- not a known variable star
07:03:44.53 -02:34:43.9 -- not a known variable star
07:03:46.87 -01:04:50.3 -- not a known variable star
07:03:48.73 -01:24:40.5 -- a known variable star
07:03:50.85 -01:11:02.4 -- not a known variable star
07:03:51.49 -02:54:47.5 -- not a known variable star
07:03:52.72 -06:00:22.1 -- not a known variable star
07:03:52.92 +00:49:49.7 -- not a known variable star
07:03:53.59 +01:24:55.8 -- not a known variable star
07:04:10.15 -05:04:53.2 -- not a known variable star
07:04:10.46 -04:42:09.2 -- not a known variable star
07:04:15.82 -02:22:56.6 -- not a known variable star
07:04:16.87 -03:01:37.5 -- not a known variable star
07:04:18.10 -00:12:34.6 -- not a known variable star
07:04:19.83 +00:50:07.3 -- not a known variable star
07:04:20.04 +02:37:45.2 -- a known variable star
07:04:20.46 -02:13:19.9 -- not a known variable star
07:04:22.70 +00:59:49.8 -- not a known variable star
07:04:34.81 -03:53:31.6 -- not a known variable star
07:04:34.96 -05:56:29.3 -- a known variable star
07:04:40.36 -01:02:13.7 -- not a known variable star
07:04:46.61 +02:30:42.1 -- not a known variable star
07:04:50.40 -01:48:49.9 -- not a known variable star
07:04:51.68 -02:12:03.7 -- not a known variable star
07:05:05.62 +02:17:06.7 -- not a known variable star
07:05:12.10 -03:19:35.2 -- not a known variable star
07:05:14.45 +00:02:10.5 -- not a known variable star
07:05:15.99 -05:50:52.5 -- not a known variable star
07:05:20.12 -02:51:44.2 -- a known variable star
07:05:24.62 -01:37:03.9 -- not a known variable star
07:05:31.89 +02:04:00.7 -- not a known variable star
07:05:35.93 -05:43:55.7 -- not a known variable star
07:05:38.60 +01:26:03.3 -- not a known variable star
07:05:41.38 -03:03:49.3 -- not a known variable star
07:05:44.24 -02:20:49.5 -- not a known variable star
07:05:45.73 -02:32:43.8 -- a known variable star
07:05:47.20 +00:13:23.9 -- a known variable star
07:05:47.79 +00:29:04.8 -- not a known variable star
07:05:50.92 -02:05:11.4 -- not a known variable star
07:06:13.57 -05:05:05.3 -- not a known variable star
07:06:26.93 -02:45:27.7 -- not a known variable star
07:06:31.58 +02:11:38.1 -- not a known variable star
07:06:31.74 +01:08:40.1 -- a known variable star
07:06:37.06 -01:28:47.0 -- a known variable star
07:06:38.15 -03:18:51.8 -- a known variable star
07:06:40.26 +00:42:28.4 -- not a known variable star
07:06:44.65 -01:25:53.6 -- not a known variable star
07:06:45.74 -01:30:47.8 -- a known variable star
07:06:45.92 -02:11:02.4 -- a known variable star
07:06:46.71 -01:31:18.8 -- not a known variable star
07:06:54.26 +02:10:49.8 -- a known variable star
07:07:11.77 -02:35:01.6 -- not a known variable star
07:07:15.74 +02:06:37.0 -- a known variable star
07:07:16.70 +01:31:11.8 -- not a known variable star
07:07:21.15 +00:33:34.9 -- not a known variable star
07:07:24.10 -01:20:23.6 -- a known variable star
07:07:24.48 +02:31:26.3 -- not a known variable star
07:07:26.03 -02:04:10.9 -- a known variable star
07:07:29.49 +01:15:34.1 -- not a known variable star
07:07:33.33 -03:25:29.3 -- a known variable star
07:07:40.35 -03:15:03.6 -- a known variable star
07:07:47.05 -02:49:20.6 -- a known variable star
07:08:04.57 -01:43:40.4 -- not a known variable star
07:08:10.79 -03:12:34.2 -- not a known variable star
07:08:21.67 -02:47:08.8 -- not a known variable star
07:08:35.63 +01:46:44.5 -- not a known variable star
07:08:43.25 +01:18:05.6 -- a known variable star
07:08:45.34 +00:41:48.8 -- a known variable star
07:08:46.29 -02:21:32.3 -- not a known variable star
07:08:47.42 -00:37:49.3 -- not a known variable star
07:08:52.68 -03:55:18.7 -- a known variable star
07:08:53.87 +00:51:37.1 -- not a known variable star
07:08:57.78 -03:05:11.8 -- a known variable star
07:08:58.19 -02:02:48.7 -- not a known variable star
07:09:03.94 -01:19:31.7 -- not a known variable star
07:09:05.02 -02:57:17.9 -- a known variable star
07:09:13.72 -02:21:30.7 -- a known variable star
07:09:14.75 -04:55:03.5 -- not a known variable star
07:09:19.51 -00:22:15.1 -- not a known variable star
07:09:20.66 +02:38:45.4 -- not a known variable star
07:09:21.65 +01:07:27.7 -- a known variable star
07:09:25.19 -03:13:04.6 -- not a known variable star
07:09:25.87 -02:13:07.3 -- not a known variable star
07:09:28.93 -06:44:36.9 -- not a known variable star
07:09:31.15 -03:28:26.8 -- not a known variable star
07:09:32.63 -07:02:49.6 -- not a known variable star
07:09:37.91 -00:01:16.9 -- a known variable star
07:09:39.99 +01:41:30.4 -- not a known variable star
07:09:40.33 -02:29:08.6 -- not a known variable star
07:09:40.95 -04:22:45.2 -- not a known variable star
07:09:41.50 -00:55:18.0 -- not a known variable star
07:09:46.21 -00:21:13.3 -- not a known variable star
07:09:53.16 -04:01:41.0 -- not a known variable star
07:09:53.98 -00:44:32.2 -- a known variable star
07:09:54.20 -04:46:45.0 -- a known variable star
07:09:56.52 -04:34:52.0 -- not a known variable star
07:09:57.99 +00:39:43.3 -- not a known variable star
07:10:06.16 +01:43:43.3 -- not a known variable star
07:10:10.13 -00:55:09.9 -- not a known variable star
07:10:10.18 -00:03:45.3 -- not a known variable star
07:10:10.81 -02:02:45.9 -- not a known variable star
07:10:12.62 +01:37:54.7 -- a known variable star
07:10:18.75 -01:17:09.9 -- not a known variable star
07:10:24.17 -06:40:08.5 -- not a known variable star
07:10:24.71 +02:20:19.3 -- not a known variable star
07:10:31.33 -00:55:56.3 -- a known variable star
07:10:32.61 -05:43:17.1 -- a known variable star
07:10:33.35 -03:53:37.9 -- not a known variable star
07:10:37.59 -04:15:17.2 -- not a known variable star
07:10:41.28 -05:05:03.5 -- a known variable star
07:10:48.74 -05:12:39.3 -- not a known variable star
07:10:56.75 -04:18:47.4 -- not a known variable star
07:11:11.54 -00:11:45.1 -- a known variable star
07:11:19.91 -03:51:45.1 -- a known variable star
07:11:22.90 -03:40:07.3 -- not a known variable star
07:11:24.98 -05:58:01.4 -- not a known variable star
07:11:44.10 -02:16:15.2 -- not a known variable star
07:11:46.28 +01:10:54.4 -- not a known variable star
07:12:04.38 -02:55:01.6 -- not a known variable star
07:12:17.29 -02:11:00.1 -- not a known variable star
07:12:18.57 -03:48:49.1 -- a known variable star
07:12:23.96 -02:24:26.6 -- not a known variable star
07:12:26.26 -04:38:59.7 -- not a known variable star
07:12:39.39 -00:37:46.5 -- not a known variable star
07:12:41.75 -00:50:01.0 -- not a known variable star
07:12:42.54 -04:10:12.5 -- a known variable star
07:12:45.14 +01:18:47.2 -- a known variable star
07:12:49.07 -03:33:13.0 -- not a known variable star
07:12:49.34 -01:30:06.5 -- not a known variable star
07:12:49.59 -00:29:11.3 -- a known variable star
07:12:56.48 -03:02:53.3 -- a known variable star
07:13:04.82 -05:12:23.7 -- a known variable star
07:13:09.03 +02:42:09.3 -- not a known variable star
07:13:31.49 -03:31:15.0 -- not a known variable star
07:13:32.71 -00:55:41.4 -- not a known variable star
07:13:39.12 -01:41:16.3 -- not a known variable star
07:13:48.38 +02:30:37.2 -- not a known variable star
07:13:59.20 -01:53:59.9 -- not a known variable star
07:14:00.02 -02:51:46.6 -- not a known variable star
07:14:23.44 -03:02:00.2 -- not a known variable star
07:14:42.78 -02:55:32.3 -- not a known variable star
07:15:17.25 -00:21:06.3 -- a known variable star
07:15:26.05 -01:11:22.1 -- not a known variable star
07:15:27.88 -02:44:52.5 -- not a known variable star
07:15:43.74 -05:23:23.8 -- not a known variable star
07:15:56.84 -02:38:27.4 -- not a known variable star
07:16:08.24 +00:05:32.3 -- not a known variable star
07:16:13.34 -00:00:45.0 -- not a known variable star
07:16:37.63 -05:50:18.1 -- not a known variable star
07:17:13.61 -02:22:29.0 -- not a known variable star
07:17:27.14 -00:59:54.5 -- not a known variable star
07:17:28.58 -01:37:03.7 -- a known variable star
07:17:31.25 +01:05:39.0 -- a known variable star
07:17:36.46 -00:24:01.1 -- a known variable star
07:17:50.85 -01:41:23.2 -- a known variable star
07:17:52.78 +00:17:04.5 -- a known variable star
07:18:05.05 -01:25:37.6 -- not a known variable star
07:18:13.69 -00:07:39.7 -- not a known variable star
07:18:14.13 -05:37:45.6 -- not a known variable star
07:18:20.90 -04:33:02.4 -- a known variable star
07:18:22.73 +00:37:23.0 -- a known variable star
07:18:29.90 -00:11:36.0 -- not a known variable star
07:18:32.61 -01:20:52.4 -- not a known variable star
07:18:36.19 -02:04:59.2 -- not a known variable star
07:18:39.14 -01:16:48.8 -- a known variable star
07:18:41.82 +01:11:02.2 -- a known variable star
07:18:48.74 -01:43:48.1 -- not a known variable star
07:18:50.17 -05:15:14.2 -- not a known variable star
07:18:52.05 -03:35:10.6 -- not a known variable star
07:19:02.10 -06:31:29.9 -- not a known variable star
07:19:02.35 -07:07:53.3 -- not a known variable star
07:19:04.11 +00:51:17.9 -- a known variable star
07:19:10.41 -01:27:06.6 -- a known variable star
07:19:10.42 -01:30:56.3 -- not a known variable star
07:19:12.60 -01:22:35.5 -- not a known variable star
07:19:23.84 +00:34:10.6 -- not a known variable star
07:19:24.04 -02:42:21.0 -- not a known variable star
07:19:26.13 +00:51:16.4 -- not a known variable star
07:19:27.26 -01:40:46.3 -- not a known variable star
07:19:50.28 -02:33:24.7 -- a known variable star
07:19:52.56 +00:18:03.9 -- not a known variable star
07:19:54.20 -01:00:37.0 -- not a known variable star
07:20:03.74 -01:48:50.7 -- not a known variable star
07:20:06.00 -02:24:28.4 -- not a known variable star
07:20:15.64 -06:40:49.0 -- not a known variable star
07:20:41.08 -03:34:37.4 -- not a known variable star
07:20:43.53 -02:48:18.5 -- not a known variable star
07:20:44.76 -05:00:17.0 -- not a known variable star
07:20:50.53 -00:51:20.8 -- a known variable star
07:20:57.72 -02:33:20.3 -- a known variable star
07:21:08.26 -01:43:14.9 -- not a known variable star
07:21:19.45 -02:07:51.0 -- not a known variable star
07:21:21.23 +00:37:45.0 -- not a known variable star
07:21:37.13 +02:27:48.5 -- not a known variable star
07:21:49.99 +00:09:23.1 -- not a known variable star
07:22:02.45 +00:44:40.0 -- not a known variable star
07:22:26.05 +00:56:45.9 -- not a known variable star
Found 316 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
438 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 438 (excluding asteroids and hot pixels, 316 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)2461149.61372226 -observatory V36
00:24:12.07 -00:14:57.4 Mercury (-0.1mag)
03:23:57.65 +18:59:11.6 Venus (-3.9mag)
00:26:40.62 +01:50:07.5 Mars (1.2mag)
07:14:05.82 +22:43:47.7 Jupiter (-2.1mag)
00:30:33.66 +00:57:33.7 Saturn (0.9mag)
03:48:21.66 +19:49:35.9 Uranus (5.8mag)
00:11:14.60 -00:12:50.1 Neptune (7.8mag)
20:33:52.86 -22:52:46.6 Pluto (14.5mag)
03:05:47.42 +22:14:12.3 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 362 Apr 18 21:47 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461149.61372226:
07:13:58.48 +22:44:02.5 Io (5.8mag)
07:13:59.68 +22:44:03.4 Europa (5.9mag)
07:13:46.46 +22:44:28.8 Ganymede (5.4mag)
07:14:22.04 +22:43:05.5 Callisto (6.6mag)
07:17:17.55 +22:30:00.9 Himalia (15.4mag)
07:14:06.89 +22:43:47.4 Thebe (16.2mag)
07:17:32.76 +23:00:20.5 Elara (17.3mag)
07:13:11.41 +23:22:10.3 Pasiphae (17.4mag)
07:22:21.25 +22:42:06.6 Carme (18.5mag)
00:30:24.81 +00:57:55.7 Titan (8.8mag)
00:30:33.09 +00:57:49.7 Rhea (10.1mag)
00:30:08.98 +00:57:13.0 Iapetus (11.5mag)
00:30:29.89 +00:58:01.7 Hyperion (14.8mag)
00:32:08.03 +01:06:01.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 18 21:47 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461149.61372226:
15:51:31.61 -18:19:44.5 JWST
16:03:50.32 +50:14:44.9 Chandra
16:56:49.84 -51:22:10.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 18 21:47 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461149.61372226 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:09.81 -28:57:56.1 13.9mag P/2010 H2 (Vales)
05:09:00.92 -69:31:03.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:08.82 +31:27:33.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:04.54 +10:54:47.9 17.6mag C/2021 G2 (ATLAS)
23:11:00.86 +29:21:19.2 17.1mag C/2022 E2 (ATLAS)
04:32:53.14 +26:07:17.8 16.0mag C/2022 N2 (PANSTARRS)
09:04:09.45 +32:01:47.0 16.2mag C/2022 QE78 (ATLAS)
08:31:36.25 +00:10:14.3 17.4mag C/2022 R6 (PANSTARRS)
18:52:55.98 +18:47:27.0 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:37.65 -11:28:32.6 17.5mag P/2023 B1 (PANSTARRS)
09:06:16.68 -11:23:31.6 17.7mag C/2023 F3 (ATLAS)
21:57:13.29 +63:05:35.7 17.5mag C/2023 H5 (Lemmon)
19:16:20.13 -03:47:22.4 14.1mag C/2023 R1 (PANSTARRS)
21:24:30.65 +86:20:50.8 17.8mag C/2023 X2 (Lemmon)
06:19:29.42 +63:30:11.5 17.2mag C/2024 A1 (ATLAS)
05:19:50.03 +19:17:35.8 11.3mag C/2024 E1 (Wierzchos)
16:17:13.02 +06:53:55.2 17.4mag C/2024 G6 (ATLAS)
20:21:36.67 +16:07:44.7 14.6mag C/2024 J3 (ATLAS)
03:29:11.32 -21:55:04.3 16.3mag C/2024 T5 (ATLAS)
05:19:23.30 +44:31:53.9 17.7mag C/2025 J1 (Borisov)
13:26:01.17 +47:19:40.7 15.3mag C/2025 L1 (ATLAS)
03:30:16.52 -26:42:28.5 17.9mag C/2025 Q3 (ATLAS)
00:17:31.19 +17:02:51.3 8.1mag C/2025 R3 (PANSTARRS)
12:52:46.97 +03:11:51.4 17.4mag C/2025 Y1 (ATLAS)
03:51:04.33 +02:20:11.5 14.2mag C/2026 A1 (MAPS)
00:08:17.06 +37:46:21.0 14.7mag C/2026 B2 (Sun-Gao)
18:48:59.20 -09:33:00.5 11.6mag 10P/Tempel
14:56:03.70 +02:52:09.6 14.3mag 24P/Schaumasse
11:02:01.23 -01:25:45.6 15.7mag 29P/Schwassmann-Wachmann
10:37:33.57 -03:51:44.5 17.0mag 43P/Wolf-Harrington
01:53:30.05 +18:00:54.6 17.3mag 47P/Ashbrook-Jackson
07:16:35.52 +36:20:16.0 17.0mag 63P/Wild
23:32:59.55 -11:04:51.5 15.7mag 65P/Gunn
04:11:39.38 +22:18:14.2 15.9mag 76P/West-Kohoutek-Ikemura
01:12:29.16 +08:50:14.5 14.3mag 78P/Gehrels
23:12:19.75 -08:28:11.0 14.7mag 88P/Howell
02:19:17.10 +21:27:34.2 15.1mag 93P/Lovas
05:00:45.24 +32:26:52.8 16.2mag 123P/West-Hartley
08:32:09.59 +36:55:35.8 16.2mag 124P/Mrkos
02:38:02.96 +14:42:50.9 16.4mag 128P/Shoemaker-Holt
02:53:39.61 +14:51:59.2 17.5mag 131P/Mueller
01:42:39.94 +14:16:23.4 10.5mag 141P/Machholz
01:51:07.10 +06:02:07.6 10.5mag 141P-A/Machholz
00:35:01.02 +01:51:00.8 12.4mag 141P-D/Machholz
02:21:38.74 +07:47:28.8 17.9mag 141P-I/Machholz
01:11:05.19 +00:02:40.9 15.0mag 162P/SidingSpring
14:45:55.66 +00:14:03.4 17.7mag 210P/Christensen
21:47:38.98 -10:42:07.8 17.7mag 218P/LINEAR
17:17:08.94 -13:33:18.1 16.1mag 235P/LINEAR
05:41:15.20 +34:55:16.1 16.8mag 240P/NEAT
07:40:05.59 -04:50:19.0 17.8mag 242P/Spahr
22:24:41.78 -20:08:01.8 17.8mag 260P/McNaught
02:04:35.82 +21:14:24.0 18.0mag 295P/LINEAR
15:41:22.22 +07:11:22.2 17.5mag 391P/Kowalski
07:35:27.35 +21:22:20.5 17.7mag 450P/LONEOS
05:40:27.53 +44:51:03.4 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 18 21:47 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 18 21:47 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 18 21:47 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:08:30.580 +41:56:13.61 AT 2026jje 2026-04-03.89 21.47
16:48:25.780 +33:00:44.35 AT 2026jjd 2026-04-03.85 21.29
16:46:02.450 +30:55:42.15 AT 2026jjc 2026-04-03.80 19.57
16:51:04.120 +44:26:50.06 AT 2026jjb 2026-03-30.84 21.02
12:10:02.030 +43:26:37.06 AT 2026jja 2026-03-28.87 21.46
17:56:59.910 +48:20:04.31 AT 2026jiz 2026-03-27.87 20.99
15:23:12.550 +15:30:01.81 AT 2026jiy 2026-03-27.82 21.09
12:45:41.400 +53:52:15.13 AT 2026jix 2026-03-24.70 20.56
12:05:28.040 +47:18:05.03 AT 2026jiw 2026-03-24.69 20.17
12:49:49.680 +44:27:28.62 AT 2026jiv 2026-03-24.69 21.87
12:17:57.600 +45:03:04.77 AT 2026jiu 2026-03-24.69 20.4
11:39:16.940 +45:15:03.67 AT 2026jit 2026-03-24.66 21.06
14:17:33.100 +43:22:03.41 AT 2026jis 2026-03-22.80 20.74
14:45:33.130 +38:26:13.04 AT 2026jir 2026-03-22.80 21.14
14:42:55.800 +38:18:34.13 AT 2026jiq 2026-03-22.80 21.14
12:43:36.900 +28:13:26.06 AT 2026jip 2026-03-20.69 21.81
13:50:42.590 +38:45:33.09 AT 2026jio 2026-03-29.93 20.87
19:45:48.257 -49:40:35.86 AT 2026jin 2026-04-12.35 18.142
23:14:08.648 +35:53:12.54 AT 2026jim 2026-03-28.53 17.909
07:22:52.030 +11:04:39.45 AT 2026jil 2026-04-11.54 18.4
-rw-r--r-- 1 apache apache 30K Apr 18 21:47 tns_transients_list.txt
