This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P
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 J086.9027+45.2906,2461147.6622,13.59,0.05,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 J086.9027+45.2906 20260417.1622 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
ZTF J054947.35+494302.2,2461147.6622,13.71,0.05,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
ZTF J054947.35+494302.2 20260417.1622 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 198008403347375360,2461147.6622,13.63,0.05,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 198008403347375360 20260417.1622 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.4478+49.1029,2461147.6622,13.81,0.05,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 J092.4478+49.1029 20260417.1622 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962016844026504832,2461147.6622,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962016844026504832 20260417.1622 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.3489+43.4595,2461147.6622,13.65,0.05,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 J088.3489+43.4595 20260417.1622 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 J087.5522+44.8128,2461147.6622,13.60,0.05,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 J087.5522+44.8128 20260417.1622 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,2461147.6622,13.61,0.05,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 20260417.1622 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 197083787085249024,2461147.6622,13.40,0.05,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
Gaia DR3 197083787085249024 20260417.1622 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1943+48.0623,2461147.6622,13.63,0.05,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 J089.1943+48.0623 20260417.1622 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.5836+50.3884,2461147.6622,13.62,0.05,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 J092.5836+50.3884 20260417.1622 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,2461147.6622,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.48,0.05,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 20260417.1622 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,2461147.6622,13.37,0.05,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 20260417.1622 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,2461147.6622,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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
ASASSN-V J060214.12+474700.6,2461147.6622,13.04,0.05,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
ASASSN-V J060214.12+474700.6 20260417.1622 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 J090.6317+46.4867,2461147.6622,13.09,0.05,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
ATO J090.6317+46.4867 20260417.1622 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.9393+43.2021,2461147.6622,12.95,0.05,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 J083.9393+43.2021 20260417.1622 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 209256067998937856,2461147.6622,12.99,0.05,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 209256067998937856 20260417.1622 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
ZTF J052512.97+410315.0,2461147.6622,12.69,0.05,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
ZTF J052512.97+410315.0 20260417.1622 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
ZTF J052234.19+485339.4,2461147.6622,12.87,0.05,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
ZTF J052234.19+485339.4 20260417.1622 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 195761791853371008,2461147.6622,12.92,0.05,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 195761791853371008 20260417.1622 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 211950176426827264,2461147.6622,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211950176426827264 20260417.1622 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,2461147.6622,13.04,0.05,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 20260417.1622 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
target,2461147.6622,12.98,0.05,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
target 20260417.1622 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 J083.1833+42.4993,2461147.6622,12.79,0.05,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 J083.1833+42.4993 20260417.1622 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.0152+49.4731,2461147.6622,12.70,0.05,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 J082.0152+49.4731 20260417.1622 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 192293833399060608,2461147.6622,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192293833399060608 20260417.1622 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
ATO J084.6215+41.2425,2461147.6622,12.64,0.05,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 J084.6215+41.2425 20260417.1622 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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,2461147.6622,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963105940357874176,2461147.6622,12.46,0.05,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 963105940357874176 20260417.1622 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 J083.2285+44.1845,2461147.6622,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.2285+44.1845 20260417.1622 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193457494657139712,2461147.6622,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193457494657139712 20260417.1622 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.7908+47.0566,2461147.6622,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.7908+47.0566 20260417.1622 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
ATO J087.8851+48.3378,2461147.6622,11.69,0.05,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 J087.8851+48.3378 20260417.1622 11.69CV 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
STARE aur0 543,2461147.6622,9.89,0.05,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
STARE aur0 543 20260417.1622 9.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3456+46.8139,2461147.6622,10.26,0.05,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 J084.3456+46.8139 20260417.1622 10.26CV 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 193611559426097664,2461147.6622,10.79,0.05,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 193611559426097664 20260417.1622 10.79CV 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 968776980814493824,2461147.6622,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968776980814493824 20260417.1622 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208040106922999808,2461147.6622,11.07,0.05,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
Gaia DR3 208040106922999808 20260417.1622 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461147.6622,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208934456550670592 20260417.1622 11.22CV 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 193039680238876672,2461147.6622,11.92,0.05,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
Gaia DR3 193039680238876672 20260417.1622 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
ATO J095.4512+46.7771,2461147.6622,11.93,0.05,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 J095.4512+46.7771 20260417.1622 11.93CV 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 J088.9926+46.7105,2461147.6622,11.87,0.05,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
ATO J088.9926+46.7105 20260417.1622 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
ATO J085.0114+50.0334,2461147.6622,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.0114+50.0334 20260417.1622 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4538117,2461147.6622,12.11,0.05,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
NSVS 4538117 20260417.1622 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3861+47.5396,2461147.6622,12.24,0.05,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
ATO J090.3861+47.5396 20260417.1622 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 197968717848571264,2461147.6622,12.05,0.05,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 197968717848571264 20260417.1622 12.05CV 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 208736750615473024,2461147.6622,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208736750615473024 20260417.1622 11.93CV 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 J087.0101+43.3293,2461147.6622,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.0101+43.3293 20260417.1622 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.9886+47.0957,2461147.6622,12.32,0.05,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
ATO J085.9886+47.0957 20260417.1622 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 194185229618901632,2461147.6622,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194185229618901632 20260417.1622 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212655861031529216,2461147.6622,12.34,0.05,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 212655861031529216 20260417.1622 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.4314+43.0363,2461147.6622,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.4314+43.0363 20260417.1622 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 J081.4978+48.5110,2461147.6622,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.4978+48.5110 20260417.1622 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0359 Aur,2461147.6622,12.63,0.05,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
V0359 Aur 20260417.1622 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8963+44.2568,2461147.6622,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8963+44.2568 20260417.1622 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.64,0.05,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 20260417.1622 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 J082.7523+42.9146,2461147.6622,12.59,0.05,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 J082.7523+42.9146 20260417.1622 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 J091.9030+46.9269,2461147.6622,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.9030+46.9269 20260417.1622 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.60,0.05,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
target 20260417.1622 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 967525667862574848,2461147.6622,12.84,0.05,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 967525667862574848 20260417.1622 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 J090.4006+42.8245,2461147.6622,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.4006+42.8245 20260417.1622 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461147.6622,12.80,0.05,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
ATO J090.6351+48.1884 20260417.1622 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 J082.0489+43.4659,2461147.6622,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.0489+43.4659 20260417.1622 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053838.70+415545.6,2461147.6622,12.79,0.05,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
ZTF J053838.70+415545.6 20260417.1622 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.8867+42.5604,2461147.6622,12.69,0.05,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 J081.8867+42.5604 20260417.1622 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 J084.0658+43.5403,2461147.6622,12.79,0.05,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 J084.0658+43.5403 20260417.1622 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8834+47.5321,2461147.6622,12.81,0.05,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 J083.8834+47.5321 20260417.1622 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 J089.5514+42.8423,2461147.6622,12.82,0.05,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 J089.5514+42.8423 20260417.1622 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 968835396666764416,2461147.6622,12.96,0.05,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 968835396666764416 20260417.1622 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 971033664007087744,2461147.6622,12.88,0.05,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 971033664007087744 20260417.1622 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
ATO J083.2234+48.7629,2461147.6622,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.2234+48.7629 20260417.1622 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,2461147.6622,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197945941638987264,2461147.6622,12.96,0.05,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 197945941638987264 20260417.1622 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 969197166055970560,2461147.6622,13.05,0.05,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 969197166055970560 20260417.1622 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.9230+50.9576,2461147.6622,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.9230+50.9576 20260417.1622 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 207620613173739776,2461147.6622,12.80,0.05,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 207620613173739776 20260417.1622 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 192624786395334400,2461147.6622,12.82,0.05,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 192624786395334400 20260417.1622 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
target,2461147.6622,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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
ATO J082.1639+48.2580,2461147.6622,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.1639+48.2580 20260417.1622 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
ATO J084.3195+44.0466,2461147.6622,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3195+44.0466 20260417.1622 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 J090.3023+47.5982,2461147.6622,12.97,0.05,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 J090.3023+47.5982 20260417.1622 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 J095.7693+49.1987,2461147.6622,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.7693+49.1987 20260417.1622 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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
ATO J083.5369+42.8145,2461147.6622,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5369+42.8145 20260417.1622 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 211466700549060736,2461147.6622,13.14,0.05,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 211466700549060736 20260417.1622 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 214264171664738816,2461147.6622,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214264171664738816 20260417.1622 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.4727+45.7717,2461147.6622,13.12,0.05,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 J087.4727+45.7717 20260417.1622 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 J079.7835+47.9155,2461147.6622,12.97,0.05,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 J079.7835+47.9155 20260417.1622 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
target,2461147.6622,13.11,0.05,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 20260417.1622 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0747+46.9169,2461147.6622,13.16,0.05,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 J091.0747+46.9169 20260417.1622 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461147.6622,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5805+44.4532 20260417.1622 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461147.6622,13.13,0.05,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 J087.2776+47.3006 20260417.1622 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.6267+48.6639,2461147.6622,13.34,0.05,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 J085.6267+48.6639 20260417.1622 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,2461147.6622,13.03,0.05,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
target 20260417.1622 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 197673090956515200,2461147.6622,13.21,0.05,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 197673090956515200 20260417.1622 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 197725867514471040,2461147.6622,13.25,0.05,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 197725867514471040 20260417.1622 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,2461147.6622,13.47,0.05,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
target 20260417.1622 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 196552271996570368,2461147.6622,13.21,0.05,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 196552271996570368 20260417.1622 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 J089.2314+46.6988,2461147.6622,13.29,0.05,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 J089.2314+46.6988 20260417.1622 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 196588835052997760,2461147.6622,13.15,0.05,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 196588835052997760 20260417.1622 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461147.6622,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.1629+50.0440 20260417.1622 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 196104946858002176,2461147.6622,13.27,0.05,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 196104946858002176 20260417.1622 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
NSV 2881,2461147.6622,13.43,0.05,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
NSV 2881 20260417.1622 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
ASASSN-V J053745.20+455814.5,2461147.6622,13.23,0.05,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
ASASSN-V J053745.20+455814.5 20260417.1622 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963318524057490944,2461147.6622,13.32,0.05,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 963318524057490944 20260417.1622 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5567+44.2856,2461147.6622,13.13,0.05,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 J083.5567+44.2856 20260417.1622 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.31,0.05,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
target 20260417.1622 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.8530+42.8735,2461147.6622,13.41,0.05,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 J087.8530+42.8735 20260417.1622 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,2461147.6622,13.54,0.05,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 20260417.1622 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,2461147.6622,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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 J091.3234+48.2792,2461147.6622,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.3234+48.2792 20260417.1622 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1559+40.9633,2461147.6622,13.31,0.05,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 J090.1559+40.9633 20260417.1622 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.4764+41.1298,2461147.6622,13.27,0.05,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 J085.4764+41.1298 20260417.1622 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 210103654024515072,2461147.6622,13.51,0.05,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 210103654024515072 20260417.1622 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.55,0.05,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 20260417.1622 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211249448220214656,2461147.6622,13.58,0.05,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 211249448220214656 20260417.1622 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
ZTF J060033.67+471756.0,2461147.6622,13.40,0.05,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 J060033.67+471756.0 20260417.1622 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 970639076772669952,2461147.6622,13.54,0.05,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 970639076772669952 20260417.1622 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 J091.6856+46.6445,2461147.6622,13.63,0.05,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 J091.6856+46.6445 20260417.1622 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 968434723461324032,2461147.6622,13.65,0.05,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 968434723461324032 20260417.1622 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 J089.8999+48.2678,2461147.6622,13.65,0.05,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 J089.8999+48.2678 20260417.1622 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,2461147.6622,13.77,0.05,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 20260417.1622 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.55,0.05,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 20260417.1622 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 J083.5685+50.2412,2461147.6622,13.55,0.05,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 J083.5685+50.2412 20260417.1622 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.57,0.05,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 20260417.1622 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 197871479789423488,2461147.6622,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197871479789423488 20260417.1622 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J094.2481+49.8491,2461147.6622,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J094.2481+49.8491 20260417.1622 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963577325904084608,2461147.6622,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963577325904084608 20260417.1622 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.3081+48.2172,2461147.6622,13.85,0.05,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 J092.3081+48.2172 20260417.1622 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 J084.8293+50.8313,2461147.6622,13.55,0.05,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 J084.8293+50.8313 20260417.1622 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 J083.6715+49.2308,2461147.6622,13.73,0.05,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 J083.6715+49.2308 20260417.1622 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 J083.1470+47.6320,2461147.6622,13.64,0.05,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 J083.1470+47.6320 20260417.1622 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 198142165807796224,2461147.6622,13.84,0.05,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 198142165807796224 20260417.1622 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.2786+48.3947,2461147.6622,13.60,0.05,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 J086.2786+48.3947 20260417.1622 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 196612577632612096,2461147.6622,13.65,0.05,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 196612577632612096 20260417.1622 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968357899382262912,2461147.6622,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968357899382262912 20260417.1622 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 J080.7222+49.0179,2461147.6622,13.41,0.05,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 J080.7222+49.0179 20260417.1622 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 969546815049439360,2461147.6622,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 969546815049439360 20260417.1622 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.60,0.05,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 20260417.1622 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 210110109360042240,2461147.6622,13.64,0.05,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 210110109360042240 20260417.1622 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 197321075438633984,2461147.6622,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197321075438633984 20260417.1622 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.3650+48.6832,2461147.6622,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.3650+48.6832 20260417.1622 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197829737003759872,2461147.6622,13.65,0.05,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 197829737003759872 20260417.1622 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963045020540085504,2461147.6622,13.88,0.05,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
Gaia DR3 963045020540085504 20260417.1622 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 J089.1696+46.8081,2461147.6622,13.60,0.05,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 J089.1696+46.8081 20260417.1622 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,2461147.6622,13.77,0.05,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 20260417.1622 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 209617876043883136,2461147.6622,13.74,0.05,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
Gaia DR3 209617876043883136 20260417.1622 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,2461147.6622,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 13.95CV 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
target,2461147.6622,13.86,0.05,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
target 20260417.1622 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209955941509956992,2461147.6622,13.77,0.05,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
Gaia DR3 209955941509956992 20260417.1622 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6622,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210417736392951936,2461147.6622,13.89,0.05,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
Gaia DR3 210417736392951936 20260417.1622 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
target,2461147.6622,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1622 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
VY Aur,2461147.6622,11.49,0.05,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
VY Aur 20260417.1622 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461147.66257141 17.04.2026 03:53:56.170 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 6 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): 22990
Objects passed selection criteria: 22960
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 20142
Average stars matched: 19699.8 (97.8043 %)
Memory usage VmPeak: 126876 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 Thu Apr 16 23:00:24 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: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461147.66257141 17.04.2026 03:53:56.170 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 541
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 106 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): 163227
Objects passed selection criteria: 162876
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: 152558
Average stars matched: 147771 (96.8619 %)
Memory usage VmPeak: 1934916 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 Thu Apr 16 23:03:51 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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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: 2461147.66183569
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Image size: 941.5'x626.6' 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: 06:00:13.336 +45:58:03.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:13.336 +45:58:03.95
Angular distance between the image centers 0.0850 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Image size: 941.5'x626.6' 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: 06:00:10.722 +45:58:02.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:10.722 +45:58:02.77
Angular distance between the image centers 0.0787 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 06:00:13.336 +45:58:03.95
Second-epoch second image center 06:00:10.722 +45:58:02.77
Angular distance between the image centers 0.00758 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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.5AhFZ5JmEC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.vBYeVEg0Oa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits &> /tmp/tmp.XfO6PqJNu8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits &> /tmp/tmp.BAvCVjKHJF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 24266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9190 to 102.4864 deg, Dec +39.9773 to +51.3461 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 77.9190 to 102.4864 deg, Dec 39.9773 to 51.3461 deg
Loaded 11816 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): 86 out of 101 total matches.
Matched with Tycho-2 101 out of 24266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 23.040760
a=0.000000 b=1.000000 c=23.040760
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
2.2 pix fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
15.0 mag. fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
15.0 mag. fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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.5AhFZ5JmEC (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2260, passed=24266
Got 24266 stars (including 21982 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 417 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 363 matched stars entering correct_measured_positions(), 321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.91"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 354 matched stars entering correct_measured_positions(), 9707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 406 matched stars entering correct_measured_positions(), 9733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.27"
Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 10903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.47"
Excluding outliers - 405 stars left (next iteration limit 389)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.vBYeVEg0Oa (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2222, passed=24282
Got 24282 stars (including 22031 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 24282 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.XfO6PqJNu8 (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1157, passed=16282
Got 16282 stars (including 15101 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 16282 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 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 15979 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 15981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 15981 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.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.BAvCVjKHJF (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1174, passed=16244
Got 16244 stars (including 15045 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 16244 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 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 15900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 649 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 15900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 15900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31730.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31502_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31502_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:42.47 +41:42:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31505_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31505_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:33:58.57 +49:58:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31508_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31508_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:54.74 +41:11:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.694 195065736570175232 079.47860479966 +41.19823177411 10.9555 10.7152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31550_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31550_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:27.53 +44:52:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)GAIADR2_OUTPUT=# 0.422 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31559_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31559_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:14:59.10 +46:47:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31579_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31579_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:43.43 +44:59:09.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31584_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31584_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:28.51 +43:00:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31606_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31606_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:23.02 +46:49:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.343 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31657_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31657_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31682_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31682_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:36.75 +45:34:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.106 962542440648583424 094.40310292280 +45.56864166395 12.1582 11.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31721_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31721_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:42:33.48 +48:14:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.711 966926674543263232 100.63972497619 +48.23720462656 12.0215 11.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31727_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31727_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:49.25 +40:57:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31730_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 31730_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:29.85 +43:09:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.764 961254401433213440 091.12410745222 +43.15702779599 12.3767 11.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:01.82 +50:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 02325_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:04.80 +50:07:24.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Image size: 941.5'x626.6' 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: 06:00:13.336 +45:58:03.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:13.336 +45:58:03.95
Angular distance between the image centers 0.0850 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Image size: 941.5'x626.6' 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: 06:00:10.722 +45:58:02.77 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:10.722 +45:58:02.77
Angular distance between the image centers 0.0787 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 06:00:13.336 +45:58:03.95
Second-epoch second image center 06:00:10.722 +45:58:02.77
Angular distance between the image centers 0.00758 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/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.RIDx2p5Wh2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.5rWNKT7Y0B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits &> /tmp/tmp.RuA4CPu9xm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits &> /tmp/tmp.G6j75xMxFj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 170851 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8948 to 102.5178 deg, Dec +39.9772 to +51.3479 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 77.8948 to 102.5178 deg, Dec 39.9772 to 51.3479 deg
Loaded 11844 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): 101 out of 140 total matches.
Matched with Tycho-2 140 out of 170851 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.801794
a=0.000000 b=1.000000 c=21.801794
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 520 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.4 mag. Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.1 mag. fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
14.1 mag. fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.RIDx2p5Wh2 (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=20120, passed=170805
Got 170805 stars (including 150422 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 170805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 406 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 356 matched stars entering correct_measured_positions(), 310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 60456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.06"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 410 matched stars entering correct_measured_positions(), 60493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.05"
Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 73193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.14"
Excluding outliers - 409 stars left (next iteration limit 387)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.5rWNKT7Y0B (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=20075, passed=170053
Got 170053 stars (including 149705 good ones) from the SExtractor catalog wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170053 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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166991 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.RuA4CPu9xm (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=11044, passed=136314
Got 136314 stars (including 125027 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat
util/solve_plate_with_UCAC5 got 136314 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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133254 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.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.G6j75xMxFj (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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=11400, passed=136496
Got 136496 stars (including 124885 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat
util/solve_plate_with_UCAC5 got 136496 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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 648 to 708 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_Aur-02-Q1b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-52-52_20.00sec_-4.90C_LIGHTs_0066.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.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_2026-04-16_CI_Aur-02-Q1b1x1_225452_TTUQ1b1x1_536452_oMS3on4P/wcs_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out195220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197613.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68332.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 218s
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: 108s
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Considering the candidate 195204_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195204_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:59.82 +45:09:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.869 197600999930098944 086.99998403289 +45.16420702399 14.7507 13.8881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195208_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195208_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:06:24.34 +44:04:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.488 961235263057938432 091.60190927977 +44.06746322477 14.7221 14.1584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195209_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195209_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:26.85 +44:45:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.247 962955032386446848 091.11228562225 +44.75885378441 14.4903 13.7425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195214_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195214_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:36.84 +46:28:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.104 197910619828145792 087.65393733063 +46.47061263701 14.5385 13.6158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195219_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195219_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:44.70 +48:44:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.685 211181725175972992 086.93691968644 +48.73478935817 14.8173 14.1159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195220_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195220_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195224_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195224_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195238_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195238_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:01:01.83 +48:38:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.745 969814580490083584 090.25833473206 +48.64796014011 14.3056 13.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195239_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195239_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195241_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195241_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195242_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195242_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195244_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195244_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195248_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195248_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:47.80 +50:23:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.710 214377043404958464 085.69887447197 +50.38382386812 14.4119 13.6273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195256_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195256_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:58.16 +45:32:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.901 197668177514416128 087.24308730609 +45.54451062165 14.6238 14.0283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195263_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195263_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:04.10 +50:05:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.000 211551161082978432 088.51749029006 +50.09856694290 14.2592 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195268_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195268_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:29.11 +50:48:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.348 214608142708363904 087.62182050965 +50.80269248900 14.4520 13.7482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195275_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195277_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195277_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195289_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195289_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:34.83 +50:07:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195290_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195290_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195293_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195293_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:51.91 +50:44:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195299_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195299_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:38.24 +42:06:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195308_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195308_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:16.37 +48:34:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.070 210989310640936320 085.31854971890 +48.57564024363 14.4697 13.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195309_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195309_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:46:55.56 +48:43:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.253 210807135307671552 086.73195235922 +48.72223729679 14.2240 13.7148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195315_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195316_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195316_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:02.67 +45:28:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195318_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195318_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195319_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195319_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:51.13 +42:23:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195323_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195323_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:47.17 +47:04:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.746 212257081908031360 080.94710958479 +47.06826294710 14.0911 13.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195327_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195327_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:20:07.65 +45:19:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.067 962335358800237952 095.03229570148 +45.32286838455 14.3073 13.7036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195333_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195333_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:16.40 +46:57:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195334_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195334_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195345_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195345_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:22.81 +50:13:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.535 213771040699836544 081.09553660911 +50.21893676587 14.1842 13.7432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195347_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195347_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:31:47.16 +48:29:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.068 967581128777104000 097.94736663910 +48.49931612479 14.1414 13.2210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195351_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195351_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:26.96 +43:07:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195352_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195352_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195353_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195353_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:16.65 +42:50:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195360_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195360_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:43.60 +50:23:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195361_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:35.12 +50:55:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195362_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195362_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:43.11 +45:46:48.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 195368_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195368_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195369_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195369_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:35:00.28 +50:18:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195370_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195370_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:39.02 +42:19:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195374_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195374_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195378_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195378_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:18.54 +41:01:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195379_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195379_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:36.85 +46:43:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.778 209668384859666048 086.15384962110 +46.72668476459 13.9845 13.4608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195380_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195380_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:24:03.28 +44:40:42.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195382_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:32.14 +44:46:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.091 208507438020791168 079.63499485094 +44.76780532452 13.8388 12.9895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195387_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195387_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:05.56 +48:22:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195389_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195389_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195390_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195390_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:36.99 +45:06:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.861 208625223204827520 079.40432633512 +45.10999810281 13.6220 12.6591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195391_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195391_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:44.23 +43:14:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195392_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195392_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195393_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195393_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195400_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:34.57 +50:01:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195402_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195402_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195407_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195407_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:03.86 +44:42:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195408_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195408_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:19.09 +41:34:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195410_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195411_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195411_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:44.22 +50:59:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.603 215225007387998592 085.93446186108 +50.98390711228 13.5660 12.9195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195412_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:50.63 +41:27:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195413_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195413_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195416_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195416_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:07:19.03 +43:29:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195417_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195417_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:27.70 +47:36:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195418_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195418_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:50.92 +49:51:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195419_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195419_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:29.61 +45:53:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.548 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195420_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195421_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195421_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:17.53 +40:45:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195422_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195422_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:59.23 +46:26:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 0.754 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195424_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195424_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:33:19.88 +49:59:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195427_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:32.81 +46:16:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.901 211837721303196800 079.63671201134 +46.28305578216 13.5567 13.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:15:57.48 +41:11:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195429_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195429_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:36:57.75 +44:14:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195430_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195430_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:06.38 +50:52:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195432_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195432_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:53.65 +50:04:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195433_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195433_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:31.99 +41:33:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195436_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195436_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195437_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195437_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:33.94 +45:13:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195440_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195440_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:14.48 +41:07:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195443_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195443_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:52.73 +47:59:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.599 210295003408140800 087.46995046697 +47.99851769905 13.1655 12.2207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195445_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195445_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195446_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195446_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:33.01 +44:26:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195447_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195447_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:14.75 +49:31:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195448_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195448_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:18:26.26 +45:34:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195451_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195451_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:21.82 +42:50:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195452_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195452_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195453_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195453_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:31.02 +47:10:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.088 209270842686354944 082.12954725612 +47.18122494840 13.2241 12.2315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195454_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195454_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195455_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195455_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:16:36.32 +44:32:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.043 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:53.27 +43:56:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195457_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195459_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195459_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195460_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195460_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:24.19 +42:05:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195462_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195462_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:47.21 +42:06:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195464_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195464_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:33.99 +44:21:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195465_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195465_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:19:25.28 +44:38:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195466_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195466_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:00.07 +43:23:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195470_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195470_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:23.02 +46:50:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:01.71 +46:28:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.663 209646837008031616 085.50739242992 +46.47416496998 13.1824 12.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195474_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195474_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:24.65 +42:28:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195475_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195475_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:36.55 +45:36:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195476_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195476_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:24.05 +41:20:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195477_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195477_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195478_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195478_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:07.36 +43:11:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195479_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195479_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195482_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195482_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:35.50 +49:58:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195483_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:14.20 +42:05:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195484_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195484_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:57.72 +44:20:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.538 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195490_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195490_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:47.66 +43:12:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195491_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195491_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:08:52.20 +45:49:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.153 963313271315430016 092.21755204281 +45.82393887969 12.7588 12.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195492_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195492_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:25:01.00 +43:59:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.814 207804540852448768 081.25389605455 +43.99275367593 12.2774 11.1507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195493_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195493_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195494_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195494_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:23.49 +41:49:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 0.739 192332281946145280 087.59814896658 +41.81778460403 12.4745 12.2458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195496_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195496_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:56.58 +42:54:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195497_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195497_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:54:42.15 +43:39:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 0.203 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195498_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195498_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:45.97 +43:34:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195499_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195499_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:42.51 +41:42:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195500_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195500_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:07.48 +45:19:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 0.535 197617561323923584 087.03135150238 +45.31853933119 12.1463 11.6118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195502_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195502_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:09.02 +46:13:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 0.790 197771561669756288 089.28789413872 +46.22871042011 12.0773 11.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195503_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195503_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:55.73 +47:36:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)
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Considering the candidate 195504_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195504_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:11.20 +45:21:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 1.159 208124253925168000 082.04712131692 +45.36645773512 11.3744 10.6083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195505_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195505_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195506_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195506_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:53.53 +45:57:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195584_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195584_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:28.48 +43:00:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195596_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195596_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:27.52 +42:19:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.20, MAG_FAINT_SEARCH_LIMIT=11.18)GAIADR2_OUTPUT=# 0.434 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195606_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195606_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195607_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195607_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:42.15 +43:22:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195614_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195614_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:44:52.54 +49:21:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195669_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195669_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:42.88 +43:37:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195673_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195673_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195688_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195688_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195701_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195701_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:34.52 +48:44:35.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195704_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195704_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195705_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195705_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:31:20.48 +46:01:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195716_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195716_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:48.05 +43:44:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195731_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195731_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195759_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195759_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:31.45 +50:41:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.292 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195767_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195767_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:01.47 +41:06:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195777_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195777_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:38.36 +45:26:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195788_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195788_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:23.78 +44:31:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195796_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195796_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:46:26.53 +47:55:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 1.240 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195798_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195798_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:19:04.22 +47:21:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.676 968930641861363072 094.76769800520 +47.36474567364 12.5150 12.0779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195799_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195799_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:36:59.26 +48:07:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.623 967332673508208256 099.24717563820 +48.11763216666 12.6763 12.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195808_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195808_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:06:21.35 +48:46:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.831 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195810_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195810_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:24:35.90 +41:36:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195814_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195814_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:36.54 +40:59:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195834_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195834_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:02:11.22 +46:42:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 0.688 963599006899237888 090.54702525212 +46.71599679132 12.7537 11.9893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195870_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195870_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:17.64 +45:03:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195875_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195875_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:49.03 +44:36:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195885_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195885_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195887_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195887_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195888_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195888_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195891_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195891_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:07.54 +44:53:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 1.278 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195894_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195894_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:46.64 +44:43:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.250 962063465895464192 093.44440342022 +44.72742362945 12.6467 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195901_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195904_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195904_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:23.58 +49:53:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195914_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195914_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:09.69 +47:19:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.511 212316245079377280 081.04053074053 +47.31751152611 12.7573 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195928_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195928_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:51.77 +42:57:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195932_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195932_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:50.21 +44:39:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.380 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195935_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195935_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:23.48 +48:55:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195943_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195943_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:43.79 +41:06:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195945_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195945_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:45.62 +49:44:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.291 213581817324797952 082.44055058336 +49.73508232948 12.8895 11.9903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195950_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195950_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:37.50 +45:55:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195956_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195956_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195966_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195966_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:07.69 +50:04:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.597 214356977317827200 085.53219554945 +50.07566096651 13.0436 12.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195968_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195968_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195970_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195970_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195973_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195973_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 195980_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195980_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:44.73 +46:30:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195982_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195982_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:08.21 +51:03:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195983_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 195983_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:39.81 +47:54:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.956 212586660519063680 080.66597215012 +47.91400751652 13.0455 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195995_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 195995_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196001_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196001_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:40.87 +44:01:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.892 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196011_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196011_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:40.25 +48:57:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196021_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196021_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:51.24 +41:14:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.426 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196024_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196024_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:02.42 +49:49:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.613 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196025_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196025_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:13.59 +42:56:27.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196038_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196038_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:46.11 +45:53:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.579 196952562947733504 089.44232599490 +45.88785721699 13.0324 12.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196052_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196052_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:31:06.74 +48:10:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196061_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196061_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:11.10 +43:58:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196062_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196062_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:58.20 +50:54:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196065_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196065_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:56.61 +46:08:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196067_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196067_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:42.97 +48:20:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.050 210971336200363648 085.17944784055 +48.33622155749 13.2097 12.6468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196068_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196068_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:45.27 +50:03:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.115 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196079_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196079_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:05.96 +41:55:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.639 960956566924526336 092.77506168430 +41.93017064148 13.2400 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196080_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196080_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:10.18 +50:14:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196090_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196090_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:40.65 +41:28:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196100_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196100_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:43.87 +41:18:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.200 194505771619147776 082.18314538158 +41.30272918703 13.1352 12.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196128_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196128_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:28.81 +45:52:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.453 962555020608754944 094.36996517508 +45.87230854494 13.3178 12.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196130_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196130_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:32.61 +43:42:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.381 196476989808724224 087.38596124422 +43.70900222684 13.0460 12.1905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196138_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196138_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:16.20 +46:04:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.499 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196139_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196139_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196141_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196141_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196151_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196151_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:12.06 +45:24:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.280 196872028016249856 088.30074499759 +45.40620224136 13.2360 12.5061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196153_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196153_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:58.82 +43:48:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196163_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196163_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:25.90 +48:47:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196176_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196176_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:01:46.08 +44:48:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.213 963002380105421184 090.44239523379 +44.81327039036 13.2765 12.3293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196181_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196181_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:01.03 +47:29:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 0.654 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:04.68 +42:17:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196209_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196212_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196212_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:17.72 +42:18:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196213_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196213_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:57.03 +43:05:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196214_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196214_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:01:04.61 +50:00:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.716 970368734350565760 090.26951411061 +50.00316418749 13.2862 12.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196230_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196230_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:06.53 +44:51:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.376 197250427518440192 085.77769553460 +44.85885826898 13.2594 12.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196232_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196232_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:22.43 +44:28:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196238_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196238_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:42.27 +45:31:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196248_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196248_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:03.65 +49:32:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196253_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196253_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:23.00 +42:40:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196257_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196257_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:06.72 +46:10:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196263_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196263_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196264_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196264_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:47:21.28 +48:12:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.949 966811809938774144 101.83902914628 +48.20028332730 13.7067 13.2028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196266_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196266_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:18.03 +43:17:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196269_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196269_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:34.76 +46:23:46.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196272_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196272_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:41.06 +48:21:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196279_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196279_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196280_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196280_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:50.31 +42:19:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196283_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196283_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:15:42.68 +42:02:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196287_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196287_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:48.10 +42:30:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196289_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:56.54 +46:11:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.814 208282721033602560 083.48553101272 +46.19874907056 13.4787 12.6535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196291_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196292_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196293_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196293_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:14.26 +50:00:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196297_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196297_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 196298_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196298_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:44.78 +44:40:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.665 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196303_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196303_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196307_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196307_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:51.33 +48:55:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.563 210461201461752192 089.21406534870 +48.93146143301 13.6447 13.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196309_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196309_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196310_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196310_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:15:16.30 +42:09:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196313_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:42.65 +47:53:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.126 212586385641158912 080.67776024297 +47.89856027064 13.3715 12.5283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196315_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196315_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196317_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196318_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196318_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:06.16 +45:12:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196325_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196325_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:30:43.57 +50:13:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196330_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196330_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:57.49 +43:06:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.466 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196341_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196341_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196345_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196345_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:38.63 +41:49:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196347_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196347_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:09.27 +46:12:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.221 209019462542689408 082.53951456145 +46.21579217952 13.5370 12.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196348_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196348_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:15.05 +40:57:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196351_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196351_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196381_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196381_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196391_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196391_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196392_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196392_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196400_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196400_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:22.04 +42:59:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.232 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196403_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196403_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:31.10 +44:15:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.923 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196406_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196410_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196410_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:24.42 +42:59:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.405 196202631594451072 084.60192928338 +42.99621569189 13.6634 13.0981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196422_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196422_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196425_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196425_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:01.85 +42:43:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.292 195300447945544064 080.50775878561 +42.71881683081 13.4492 12.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196427_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196427_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:47.46 +47:00:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.439 212303050943149440 080.69756548932 +47.01475255644 13.7614 13.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196429_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196429_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:47:20.91 +48:12:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196432_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196432_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:58.03 +43:42:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.840 207515987770326784 079.74275755653 +43.70229955072 13.6619 12.7892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196437_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196437_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:28.36 +42:00:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.334 195912429244634624 084.36928975315 +42.01213215946 13.8357 13.3198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196438_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196438_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:14.01 +47:43:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.996 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196443_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196443_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196444_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196444_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196447_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196447_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196454_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196454_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:40.36 +42:51:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:37.84 +43:07:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196460_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196460_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196465_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196465_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196467_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196467_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:26.02 +44:48:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.668 208051140694611328 081.85896515545 +44.81408172898 13.6708 13.3725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196470_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196470_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:47.41 +41:40:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196472_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196472_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:31.25 +47:51:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.583 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196474_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196474_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:05.77 +48:44:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196475_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196475_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196476_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196476_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196479_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:45.41 +45:22:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196482_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196482_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:18.12 +46:15:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196488_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196488_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:50.40 +45:03:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.123 208529600051866240 079.96005250816 +45.06203311659 13.7148 12.6649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196489_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196489_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:02.54 +46:44:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196492_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196492_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:27.59 +46:35:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196497_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196497_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:02.95 +49:04:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196504_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196504_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:21.80 +47:52:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196507_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196507_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196509_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196509_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196512_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196512_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:33.87 +45:29:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196513_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196513_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:43.64 +50:12:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196515_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196527_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196527_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196530_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196530_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196532_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196532_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:23.98 +43:46:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.007 195777429833427968 083.35022209389 +43.77985576823 13.6692 12.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196534_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196534_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:30.24 +43:50:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.479 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196535_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196535_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:41.47 +50:41:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.248 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196538_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196538_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:51.14 +46:21:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196540_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196540_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196542_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196542_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:29.94 +44:44:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.707 197245582797409152 085.62447289270 +44.74687417395 12.5370 11.1711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196545_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196545_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:30.38 +41:38:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196547_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196547_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:20.03 +45:58:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.409 208252729279086464 082.83335404737 +45.97527379616 13.9254 13.0817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196550_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196550_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:57.50 +42:25:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196554_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196554_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:59.21 +46:57:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196555_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196555_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196557_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196557_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196559_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196561_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196561_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:34:27.95 +50:19:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196563_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196563_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196564_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196564_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:33.33 +49:50:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196569_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196569_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:56.74 +47:43:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.442 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196572_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196572_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:48.36 +48:50:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196573_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196573_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:23.17 +49:46:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.077 211485637061247744 087.09740055049 +49.78256265660 13.8223 13.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196576_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196576_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:50.71 +42:45:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196577_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196577_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:09.99 +42:09:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196583_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196583_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196590_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196590_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:59.10 +43:51:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196608_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196608_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:32.62 +41:57:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196613_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196613_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:08.64 +50:16:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196620_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196620_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:25:05.01 +42:33:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196621_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196621_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:52:21.10 +42:50:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196624_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196624_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:17.38 +45:05:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196626_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196626_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:16:56.63 +44:02:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196627_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196627_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:41.81 +41:30:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196628_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196628_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:25.33 +42:00:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196632_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196632_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:13:29.78 +47:17:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.990 968785712485462016 093.37489471116 +47.29624681696 14.0869 13.4852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196644_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196644_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:54.13 +46:06:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196652_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196652_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:46:39.76 +43:21:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196657_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196657_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:53.30 +46:05:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.019 197005378160950784 089.47179707530 +46.09439219961 14.0011 13.1854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196658_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196658_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:40:34.17 +46:53:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196660_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196660_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:13.41 +46:47:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196661_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196661_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:49.02 +51:04:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196663_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196663_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196666_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196666_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:43.08 +50:10:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.247 213769219633738112 080.92960190688 +50.17639561905 13.7633 12.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196667_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196667_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:50.52 +44:16:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196674_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196674_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:38:01.48 +48:29:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196683_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196683_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:50.51 +49:49:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196685_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196685_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:37.11 +49:04:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196686_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196686_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196687_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196687_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:44.66 +49:34:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.949 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196692_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196692_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:24:24.81 +44:48:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.188 208086290707268608 081.10372106703 +44.80994290569 13.9169 13.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196694_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196694_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:18.63 +47:12:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.568 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196701_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196701_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196702_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196702_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:32.00 +48:16:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196703_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196703_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:22:55.57 +50:29:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196704_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:27.84 +47:51:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196708_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196708_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:51.06 +49:26:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196718_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196718_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196736_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196736_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196738_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196738_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:03.98 +44:57:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196739_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196739_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196743_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196743_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:39.56 +43:01:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196745_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196745_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:07.35 +44:31:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.675 207889134528538624 082.78166691688 +44.52814416897 13.9498 13.1061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196748_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196748_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:55:48.18 +42:30:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196753_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196753_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196762_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196762_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:44.95 +47:30:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.451 968792721871861888 093.18747696802 +47.51186298846 14.0070 13.4569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196768_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196768_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:57.28 +42:41:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196771_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196771_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:17:15.33 +42:06:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196776_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196776_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:20:02.70 +46:37:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196780_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196780_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:12.75 +49:06:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.988 970669347702108288 096.55228667167 +49.11057778149 13.8025 12.7263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196783_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196783_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:17:45.69 +44:42:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196785_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196785_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:00.81 +46:20:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.313 208287501334038656 083.50390290064 +46.33909529807 14.0153 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196787_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196787_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196792_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196792_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:48.91 +46:10:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.550 208974588724407424 081.95398429282 +46.17604659977 13.9532 13.0798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196793_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196793_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:43.67 +46:56:37.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196794_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196794_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:05.36 +46:34:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196803_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196803_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:35:41.20 +44:16:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196804_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196804_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:21.17 +42:41:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196805_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196805_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:56.39 +50:48:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.545 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196807_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196807_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:12:20.06 +50:12:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.654 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196815_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196815_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196816_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196816_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196826_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196826_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:47:28.60 +41:25:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196829_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196829_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:11:51.77 +45:03:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.691 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196831_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196831_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:19:44.15 +47:47:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.648 212218358483551616 079.93457606840 +47.79294561915 13.8506 12.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196833_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196833_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:26:28.24 +42:41:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196835_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196835_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:50.46 +43:25:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.152 207403150388969728 080.20981679218 +43.43177546007 13.8634 12.9877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196836_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196836_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:08.64 +44:09:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.649 196559904153704320 087.28692386633 +44.15359747280 14.2789 13.4781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196838_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196838_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:23:09.86 +49:09:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.974 970593653198168064 095.79099454777 +49.16629137386 14.1385 13.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196839_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196839_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:58.76 +46:09:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196849_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196849_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:11.35 +42:50:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.898 192511364902195840 089.29695470380 +42.84027162771 14.0339 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196858_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196858_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196860_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196860_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:24.74 +49:14:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196861_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196861_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:25.51 +42:20:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.261 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196862_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196862_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196866_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196866_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:55.67 +45:00:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196870_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196870_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:32.48 +47:01:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.352 209826096057773184 084.88628198768 +47.01913001902 14.1003 13.2484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196872_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196872_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:44.67 +42:36:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.727 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196873_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196873_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:51:57.07 +41:37:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.697 192277649962098688 087.98771623166 +41.62337032686 13.8897 13.1157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196876_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196876_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:30:02.70 +50:08:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196883_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196883_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196888_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196888_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196890_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196890_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:21:05.85 +40:34:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196893_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196893_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:24:57.26 +49:09:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.395 970672611877277184 096.23956597917 +49.15474510578 14.1813 13.5313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196902_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196902_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196906_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196906_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196908_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196908_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196909_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196909_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196914_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196914_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:23.40 +49:49:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196921_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196921_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:51.90 +48:16:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.903 212612670840480000 080.96704413027 +48.26814712789 14.0705 13.5224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196923_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196923_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:24.66 +43:50:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196924_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196924_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:58.13 +50:12:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196933_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196933_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:07.62 +50:26:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.401 214568598946171264 087.03234717596 +50.43577947810 13.9372 13.3806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196939_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196939_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196940_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196940_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:59.79 +47:35:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.664 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196944_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196944_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:48.57 +48:50:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196948_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196948_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:18:53.77 +41:48:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 2.545 195118032094510464 079.72494683518 +41.81137779987 14.0386 13.4776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196951_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196951_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196952_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196952_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:13.64 +49:41:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.164 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196953_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196953_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:36:07.16 +47:47:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.702 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196954_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196954_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:16.21 +43:16:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.811 196045745028719488 085.56775371942 +43.27358583012 14.0728 13.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196958_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196958_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196959_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196959_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:33.87 +49:48:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.116 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196978_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196978_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196983_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 196983_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:15.61 +45:20:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196985_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196985_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196992_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196992_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 196993_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 196993_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197002_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197002_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:19.37 +44:51:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.865 197388557964679936 084.33047764237 +44.86089830184 14.1156 13.5024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197010_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197010_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:58:09.56 +48:37:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.804 210251469618523520 089.54055114472 +48.62003298825 14.3909 13.8430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197011_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197011_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:42:47.44 +45:58:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197022_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197022_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:31.21 +41:51:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197024_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197024_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:38.70 +47:49:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.002 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197033_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197033_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197036_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197036_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197042_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197042_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:32.15 +47:15:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.812 210597025508196480 084.63478085416 +47.26331477231 14.1422 13.2923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197051_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197051_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:53.78 +46:32:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.749 209184908981247744 081.97518253378 +46.54961465738 14.0914 13.2181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197054_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197054_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:34.83 +44:30:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197055_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197055_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:59.85 +45:05:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197058_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197058_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197082_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197082_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:56:00.70 +49:05:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.046 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197086_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197086_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197088_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197088_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:50:06.57 +46:08:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197094_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197094_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:50.94 +44:37:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.266 196765718986467072 087.46228975327 +44.61842946632 14.1958 13.3664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197097_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197097_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:09:10.38 +42:04:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197103_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197103_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:00.20 +45:32:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.852 963235820168851712 092.50109436752 +45.54496087176 14.4482 13.9808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197115_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197115_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:09:37.17 +50:22:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.666 971732094409236096 092.40552932955 +50.38177186496 14.5645 13.9943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197120_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197120_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197126_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197126_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197136_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197136_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197139_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197139_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197155_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197155_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197164_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197164_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:31:09.08 +50:39:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.811 213847353679179392 082.78816156270 +50.65301417970 14.2713 13.7490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197173_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197173_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197174_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197174_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197181_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197181_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:53:58.40 +42:30:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:41:07.51 +47:58:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197220_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197220_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197226_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197226_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197232_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197232_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 197247_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197247_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197250_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197250_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:42:04.49 +49:39:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.138 991157299479352960 100.51871738467 +49.66107312699 14.5771 14.0745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197262_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197262_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:43.01 +51:03:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.156 215182332592783104 084.67927379237 +51.05631982337 14.5071 13.7174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197264_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197264_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:13.61 +44:55:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197265_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197265_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:32:22.31 +44:33:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.998 207880127978442368 083.09323367673 +44.55836260963 14.5512 13.9367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197268_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197268_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:04:57.75 +43:08:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.090 961276666543652608 091.24098583360 +43.14171180699 14.5684 14.0056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197270_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197270_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:20:12.64 +49:24:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197274_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197274_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:03:02.69 +46:44:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.743 963597151473005312 090.76167548963 +46.73289191284 14.4883 13.8730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197278_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197278_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197279_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197279_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:00:34.66 +46:38:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197305_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197305_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:46.92 +46:28:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.479 209612206687131136 086.19689831834 +46.47272458834 14.4861 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197308_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197308_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197312_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197312_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197317_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197317_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:38:17.18 +51:03:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197329_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197329_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197330_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197330_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197337_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197337_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197360_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197360_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197361_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197361_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197370_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197370_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:01.01 +50:51:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.676 215164328089901312 084.75470819569 +50.86162018101 14.5533 13.7113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197376_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197376_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:51.46 +47:14:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.670 212312469806204544 080.96498623835 +47.23745062327 14.3911 13.5064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197379_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197379_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:45:30.73 +45:46:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.680 197511119150017024 086.37854119210 +45.77189386909 14.7959 14.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197380_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197380_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197387_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197387_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197390_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197390_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197394_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197394_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197402_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197402_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197414_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197414_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197421_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197421_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197423_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197423_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197431_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197431_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:18:59.61 +47:22:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.392 968930710580840064 094.74849015453 +47.36711863901 14.8235 14.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197436_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197436_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:23:46.10 +44:33:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.264 207704652796021504 080.94245655096 +44.55470164267 14.1923 13.2291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197446_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197446_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:38:58.61 +48:06:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.804 966959281936055168 099.74387781169 +48.10361695033 14.6826 14.0153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197453_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197453_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197456_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197468_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197468_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197471_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197491_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197491_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:41:26.51 +49:34:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.906 991162011059867264 100.36018758865 +49.58112513686 14.8928 14.2923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197494_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197494_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197517_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197517_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197522_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197522_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197528_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197528_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197529_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197529_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:10:00.34 +46:40:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.211 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197530_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197530_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:05:19.84 +49:43:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.564 970294311157627264 091.33310339506 +49.72928098849 14.6509 14.0910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197551_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197551_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197564_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197564_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:34:44.93 +48:41:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.219 213993245127650688 083.68719099883 +48.68897728729 14.7273 13.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197570_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197570_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:26.82 +50:33:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.035 214403225525499648 086.11220251936 +50.56264222298 14.7783 14.1780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197579_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197579_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:51.41 +51:05:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.042 211664376420455168 089.96466731365 +51.09810907484 14.6737 14.0602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197586_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197586_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:48:20.20 +49:24:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.060 211412622617327488 087.08486619000 +49.40706970153 14.8046 13.9184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197587_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197587_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197591_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197591_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:29:36.65 +48:08:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.674 212457845858919424 082.40318324799 +48.13661800230 14.5949 14.0236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197593_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197593_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197613_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197613_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197618_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197618_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197622_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 197622_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 197625_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197625_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:33:55.62 +50:15:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.286 215120553783587712 083.48189386714 +50.25207156569 14.7423 14.0639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197637_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197637_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:39:34.36 +42:20:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.194 195935209751002752 084.89360411427 +42.33684241881 14.4030 13.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197638_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197638_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:49:49.36 +48:59:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.757 211192548493772928 087.45641007298 +48.98506741292 15.0158 14.3477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197646_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197646_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:44:05.68 +44:24:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.048 196431604890229376 086.02397310746 +44.41485836437 14.9101 14.0831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197652_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197652_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:28:34.31 +48:03:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.653 212461792933404416 082.14281523974 +48.05906818457 14.5978 13.7896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197668_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 197668_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:43:46.21 +44:59:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.812 197258094036493824 085.94299855856 +44.99419142545 14.3799 13.2436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:26:01.78 +50:29:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:14:59.10 +46:47:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:37:56.95 +44:41:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43409_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 43409_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:57:23.96 +48:22:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:27:04.78 +50:07:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116770_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:21:29.78 +43:44:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-16_22-53-56_20.00sec_-4.90C_LIGHTs_0067 did not pass the final checks
**** FOUND 05:59:44.14 +47:37:01.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 336s
Prepared the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:47:38.43 +45:18:35.3
05:49:47.21 +49:43:02.6
05:51:55.67 +47:05:43.1
06:09:46.97 +49:06:39.5
06:13:25.90 +44:01:20.9
05:53:23.54 +43:27:35.3
05:50:10.28 +44:48:35.8
05:45:13.31 +49:30:40.2
05:42:11.17 +44:18:00.7
05:56:48.41 +48:03:55.4
06:10:20.87 +50:23:13.5
06:12:04.60 +50:30:17.1
06:14:00.15 +49:18:13.1
06:18:02.39 +43:28:06.6
05:45:51.96 +50:23:48.3
06:02:14.20 +47:47:00.4
06:02:31.73 +46:29:05.7
05:35:47.18 +43:12:13.9
05:27:18.09 +46:58:13.2
05:25:14.46 +41:03:21.2
05:22:33.99 +48:53:35.1
05:29:09.72 +43:57:13.3
05:21:49.37 +47:17:20.3
06:01:13.12 +48:48:39.5
06:23:12.82 +46:48:44.6
05:32:45.81 +42:29:58.6
05:28:04.18 +49:28:29.4
05:54:06.75 +41:46:11.9
05:38:27.34 +41:13:51.4
05:15:02.20 +48:43:56.7
06:16:43.96 +44:42:41.2
05:27:16.19 +45:33:35.1
06:05:28.41 +45:37:48.9
05:32:56.89 +44:10:54.0
05:50:14.65 +43:23:13.6
06:11:13.09 +47:02:39.1
05:51:38.20 +48:20:09.2
05:17:54.82 +41:11:53.5
05:37:22.98 +46:49:18.4
05:56:09.53 +44:18:00.2
06:15:16.63 +47:16:52.4
05:26:36.87 +44:48:50.0
05:25:37.70 +45:40:56.7
05:43:17.36 +42:28:49.5
06:21:48.26 +46:46:30.5
05:55:58.21 +46:42:37.2
05:40:02.85 +50:02:04.9
06:00:40.09 +44:34:45.4
06:01:32.31 +47:32:24.8
05:48:46.00 +46:35:02.1
05:18:23.05 +45:25:54.9
05:48:04.06 +43:19:50.8
05:43:52.77 +47:06:14.4
05:26:28.90 +41:11:31.1
05:28:01.36 +48:15:00.3
05:37:46.25 +43:03:12.9
05:56:30.92 +46:14:49.3
05:25:59.73 +48:30:07.9
05:57:46.58 +43:35:10.9
05:35:35.23 +44:15:15.1
06:01:40.58 +44:57:47.9
05:31:00.36 +42:54:52.9
06:07:29.92 +46:55:57.3
05:27:51.03 +42:20:26.2
06:25:49.06 +48:15:44.2
06:01:31.69 +42:49:21.1
06:02:32.06 +48:11:24.9
05:28:11.75 +43:27:55.8
05:38:35.64 +41:55:49.6
05:27:30.92 +42:33:45.2
05:36:14.55 +43:32:31.3
05:35:36.13 +47:32:42.8
06:46:31.34 +47:39:11.5
05:58:13.69 +42:51:14.3
06:13:33.57 +48:03:18.1
06:15:21.77 +50:34:28.5
05:32:56.19 +48:45:35.2
05:44:39.82 +43:57:55.7
05:53:28.90 +46:52:04.8
06:14:39.20 +48:05:36.3
05:19:09.74 +44:39:54.1
05:39:41.60 +50:57:35.7
05:20:50.94 +44:04:37.6
05:57:45.39 +45:54:52.3
05:40:57.37 +41:07:44.9
05:42:50.65 +48:07:39.2
05:28:41.38 +48:14:36.0
05:37:16.40 +44:02:48.7
05:53:51.87 +50:42:48.4
06:01:16.81 +47:35:44.8
06:23:05.44 +49:11:47.2
06:26:29.79 +49:54:10.6
05:34:07.90 +42:49:01.2
05:48:07.82 +49:40:40.6
05:38:36.21 +49:43:22.4
05:49:53.28 +45:46:16.6
05:57:12.15 +42:33:32.6
05:19:05.29 +47:54:37.2
05:48:08.81 +44:44:55.2
06:04:15.52 +46:54:36.4
05:34:19.08 +44:27:44.3
05:49:06.52 +47:17:59.3
05:42:31.38 +48:39:43.3
05:28:27.52 +43:54:02.9
05:49:15.68 +45:41:16.2
05:52:11.39 +46:15:47.1
06:47:02.58 +49:45:30.8
05:50:28.74 +44:11:34.7
05:56:58.12 +46:41:29.5
05:52:58.21 +44:33:09.8
05:36:40.74 +50:02:54.9
05:45:51.20 +43:22:56.0
06:16:06.10 +44:42:54.1
05:37:41.41 +45:58:09.0
06:07:54.18 +45:58:50.2
05:46:44.70 +43:22:54.5
05:34:15.91 +44:17:04.7
06:36:36.45 +40:24:48.9
05:51:25.06 +42:52:21.1
06:17:15.78 +49:29:56.5
05:39:42.58 +45:03:31.2
06:05:14.62 +48:16:56.5
06:00:41.06 +40:57:37.3
05:41:56.64 +41:07:32.7
05:50:48.96 +47:35:39.5
05:59:03.69 +45:50:37.0
05:54:17.75 +49:03:40.9
06:00:34.86 +47:18:29.4
06:21:40.27 +49:12:11.0
06:06:46.95 +46:38:16.7
06:22:49.17 +46:07:41.3
05:59:31.97 +48:16:10.6
06:41:34.62 +49:47:47.5
05:41:47.36 +46:24:57.9
05:34:12.98 +50:14:24.7
06:01:32.46 +48:06:13.3
05:59:14.55 +47:08:48.0
06:16:58.55 +49:51:23.5
06:01:14.43 +46:27:30.0
06:09:09.88 +48:13:10.6
05:39:19.04 +50:49:46.9
05:34:37.86 +49:13:53.9
05:32:33.73 +47:37:16.1
05:56:55.23 +47:37:51.6
05:45:07.09 +48:23:49.9
05:54:54.39 +44:20:23.9
06:20:20.72 +45:44:41.6
05:22:53.30 +49:01:02.2
06:11:23.77 +47:36:13.7
05:37:55.68 +43:03:20.1
05:51:22.89 +47:46:01.8
05:37:17.61 +44:28:41.6
05:33:27.70 +48:41:04.7
05:53:58.22 +46:34:05.2
06:01:52.33 +45:20:53.0
05:56:41.19 +46:49:07.2
05:46:08.46 +49:03:28.6
05:45:22.39 +46:38:00.8
05:45:32.61 +50:33:19.1
05:40:47.25 +50:52:24.0
05:46:07.47 +47:42:00.8
05:46:45.05 +46:07:07.8
05:55:29.21 +48:34:00.8
05:43:36.05 +44:00:57.2
06:09:51.91 +46:34:27.5
########### Completed Aur-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 ####
05:47:38.43 +45:18:35.3
05:49:47.21 +49:43:02.6
05:51:55.67 +47:05:43.1
06:09:46.97 +49:06:39.5
06:13:25.90 +44:01:20.9
05:53:23.54 +43:27:35.3
05:50:10.28 +44:48:35.8
05:45:13.31 +49:30:40.2
05:42:11.17 +44:18:00.7
05:56:48.41 +48:03:55.4
06:10:20.87 +50:23:13.5
06:12:04.60 +50:30:17.1
06:14:00.15 +49:18:13.1
06:18:02.39 +43:28:06.6
05:45:51.96 +50:23:48.3
06:02:14.20 +47:47:00.4
06:02:31.73 +46:29:05.7
05:35:47.18 +43:12:13.9
05:27:18.09 +46:58:13.2
05:25:14.46 +41:03:21.2
05:22:33.99 +48:53:35.1
05:29:09.72 +43:57:13.3
05:21:49.37 +47:17:20.3
06:01:13.12 +48:48:39.5
06:23:12.82 +46:48:44.6
05:32:45.81 +42:29:58.6
05:28:04.18 +49:28:29.4
05:54:06.75 +41:46:11.9
05:38:27.34 +41:13:51.4
05:15:02.20 +48:43:56.7
06:16:43.96 +44:42:41.2
05:27:16.19 +45:33:35.1
06:05:28.41 +45:37:48.9
05:32:56.89 +44:10:54.0
05:50:14.65 +43:23:13.6
06:11:13.09 +47:02:39.1
05:51:38.20 +48:20:09.2
05:17:54.82 +41:11:53.5
05:37:22.98 +46:49:18.4
05:56:09.53 +44:18:00.2
06:15:16.63 +47:16:52.4
05:26:36.87 +44:48:50.0
05:25:37.70 +45:40:56.7
05:43:17.36 +42:28:49.5
06:21:48.26 +46:46:30.5
05:55:58.21 +46:42:37.2
05:40:02.85 +50:02:04.9
06:00:40.09 +44:34:45.4
06:01:32.31 +47:32:24.8
05:48:46.00 +46:35:02.1
05:18:23.05 +45:25:54.9
05:48:04.06 +43:19:50.8
05:43:52.77 +47:06:14.4
05:26:28.90 +41:11:31.1
05:28:01.36 +48:15:00.3
05:37:46.25 +43:03:12.9
05:56:30.92 +46:14:49.3
05:25:59.73 +48:30:07.9
05:57:46.58 +43:35:10.9
05:35:35.23 +44:15:15.1
06:01:40.58 +44:57:47.9
05:31:00.36 +42:54:52.9
06:07:29.92 +46:55:57.3
05:27:51.03 +42:20:26.2
06:25:49.06 +48:15:44.2
06:01:31.69 +42:49:21.1
06:02:32.06 +48:11:24.9
05:28:11.75 +43:27:55.8
05:38:35.64 +41:55:49.6
05:27:30.92 +42:33:45.2
05:36:14.55 +43:32:31.3
05:35:36.13 +47:32:42.8
06:46:31.34 +47:39:11.5
05:58:13.69 +42:51:14.3
06:13:33.57 +48:03:18.1
06:15:21.77 +50:34:28.5
05:32:56.19 +48:45:35.2
05:44:39.82 +43:57:55.7
05:53:28.90 +46:52:04.8
06:14:39.20 +48:05:36.3
05:19:09.74 +44:39:54.1
05:39:41.60 +50:57:35.7
05:20:50.94 +44:04:37.6
05:57:45.39 +45:54:52.3
05:40:57.37 +41:07:44.9
05:42:50.65 +48:07:39.2
05:28:41.38 +48:14:36.0
05:37:16.40 +44:02:48.7
05:53:51.87 +50:42:48.4
06:01:16.81 +47:35:44.8
06:23:05.44 +49:11:47.2
06:26:29.79 +49:54:10.6
05:34:07.90 +42:49:01.2
05:48:07.82 +49:40:40.6
05:38:36.21 +49:43:22.4
05:49:53.28 +45:46:16.6
05:57:12.15 +42:33:32.6
05:19:05.29 +47:54:37.2
05:48:08.81 +44:44:55.2
06:04:15.52 +46:54:36.4
05:34:19.08 +44:27:44.3
05:49:06.52 +47:17:59.3
05:42:31.38 +48:39:43.3
05:28:27.52 +43:54:02.9
05:49:15.68 +45:41:16.2
05:52:11.39 +46:15:47.1
06:47:02.58 +49:45:30.8
05:50:28.74 +44:11:34.7
05:56:58.12 +46:41:29.5
05:52:58.21 +44:33:09.8
05:36:40.74 +50:02:54.9
05:45:51.20 +43:22:56.0
06:16:06.10 +44:42:54.1
05:37:41.41 +45:58:09.0
06:07:54.18 +45:58:50.2
05:46:44.70 +43:22:54.5
05:34:15.91 +44:17:04.7
06:36:36.45 +40:24:48.9
05:51:25.06 +42:52:21.1
06:17:15.78 +49:29:56.5
05:39:42.58 +45:03:31.2
06:05:14.62 +48:16:56.5
06:00:41.06 +40:57:37.3
05:41:56.64 +41:07:32.7
05:50:48.96 +47:35:39.5
05:59:03.69 +45:50:37.0
05:54:17.75 +49:03:40.9
06:00:34.86 +47:18:29.4
06:21:40.27 +49:12:11.0
06:06:46.95 +46:38:16.7
06:22:49.17 +46:07:41.3
05:59:31.97 +48:16:10.6
06:41:34.62 +49:47:47.5
05:41:47.36 +46:24:57.9
05:34:12.98 +50:14:24.7
06:01:32.46 +48:06:13.3
05:59:14.55 +47:08:48.0
06:16:58.55 +49:51:23.5
06:01:14.43 +46:27:30.0
06:09:09.88 +48:13:10.6
05:39:19.04 +50:49:46.9
05:34:37.86 +49:13:53.9
05:32:33.73 +47:37:16.1
05:56:55.23 +47:37:51.6
05:45:07.09 +48:23:49.9
05:54:54.39 +44:20:23.9
06:20:20.72 +45:44:41.6
05:22:53.30 +49:01:02.2
06:11:23.77 +47:36:13.7
05:37:55.68 +43:03:20.1
05:51:22.89 +47:46:01.8
05:37:17.61 +44:28:41.6
05:33:27.70 +48:41:04.7
05:53:58.22 +46:34:05.2
06:01:52.33 +45:20:53.0
05:56:41.19 +46:49:07.2
05:46:08.46 +49:03:28.6
05:45:22.39 +46:38:00.8
05:45:32.61 +50:33:19.1
05:40:47.25 +50:52:24.0
05:46:07.47 +47:42:00.8
05:46:45.05 +46:07:07.8
05:55:29.21 +48:34:00.8
05:43:36.05 +44:00:57.2
06:09:51.91 +46:34:27.5
###################################################################################
05:47:38.43 +45:18:35.3 -- not an asteroid (will add it to exclusion list)
05:49:47.21 +49:43:02.6 -- not an asteroid (will add it to exclusion list)
05:51:55.67 +47:05:43.1 -- not an asteroid (will add it to exclusion list)
06:09:46.97 +49:06:39.5 -- not an asteroid (will add it to exclusion list)
06:13:25.90 +44:01:20.9 -- not an asteroid (will add it to exclusion list)
05:53:23.54 +43:27:35.3 -- not an asteroid (will add it to exclusion list)
05:50:10.28 +44:48:35.8 -- not an asteroid (will add it to exclusion list)
05:45:13.31 +49:30:40.2 -- not an asteroid (will add it to exclusion list)
05:42:11.17 +44:18:00.7 -- not an asteroid (will add it to exclusion list)
05:56:48.41 +48:03:55.4 -- not an asteroid (will add it to exclusion list)
06:10:20.87 +50:23:13.5 -- not an asteroid (will add it to exclusion list)
06:12:04.60 +50:30:17.1 -- not an asteroid (will add it to exclusion list)
06:14:00.15 +49:18:13.1 -- not an asteroid (will add it to exclusion list)
06:18:02.39 +43:28:06.6 -- not an asteroid (will add it to exclusion list)
05:45:51.96 +50:23:48.3 -- not an asteroid (will add it to exclusion list)
06:02:14.20 +47:47:00.4 -- not an asteroid (will add it to exclusion list)
06:02:31.73 +46:29:05.7 -- not an asteroid (will add it to exclusion list)
05:35:47.18 +43:12:13.9 -- not an asteroid (will add it to exclusion list)
05:27:18.09 +46:58:13.2 -- not an asteroid (will add it to exclusion list)
05:25:14.46 +41:03:21.2 -- not an asteroid (will add it to exclusion list)
05:22:33.99 +48:53:35.1 -- not an asteroid (will add it to exclusion list)
05:29:09.72 +43:57:13.3 -- not an asteroid (will add it to exclusion list)
05:21:49.37 +47:17:20.3 -- not an asteroid (will add it to exclusion list)
06:01:13.12 +48:48:39.5 -- not an asteroid (will add it to exclusion list)
06:23:12.82 +46:48:44.6 -- not an asteroid (will add it to exclusion list)
05:32:45.81 +42:29:58.6 -- not an asteroid (will add it to exclusion list)
05:28:04.18 +49:28:29.4 -- not an asteroid (will add it to exclusion list)
05:54:06.75 +41:46:11.9 -- not an asteroid (will add it to exclusion list)
05:38:27.34 +41:13:51.4 -- not an asteroid (will add it to exclusion list)
05:15:02.20 +48:43:56.7 -- not an asteroid (will add it to exclusion list)
06:16:43.96 +44:42:41.2 -- not an asteroid (will add it to exclusion list)
05:27:16.19 +45:33:35.1 -- not an asteroid (will add it to exclusion list)
06:05:28.41 +45:37:48.9 -- not an asteroid (will add it to exclusion list)
05:32:56.89 +44:10:54.0 -- not an asteroid (will add it to exclusion list)
05:50:14.65 +43:23:13.6 -- not an asteroid (will add it to exclusion list)
06:11:13.09 +47:02:39.1 -- not an asteroid (will add it to exclusion list)
05:51:38.20 +48:20:09.2 -- not an asteroid (will add it to exclusion list)
05:17:54.82 +41:11:53.5 -- not an asteroid (will add it to exclusion list)
05:37:22.98 +46:49:18.4 -- not an asteroid (will add it to exclusion list)
05:56:09.53 +44:18:00.2 -- not an asteroid (will add it to exclusion list)
06:15:16.63 +47:16:52.4 -- not an asteroid (will add it to exclusion list)
05:26:36.87 +44:48:50.0 -- not an asteroid (will add it to exclusion list)
05:25:37.70 +45:40:56.7 -- not an asteroid (will add it to exclusion list)
05:43:17.36 +42:28:49.5 -- not an asteroid (will add it to exclusion list)
06:21:48.26 +46:46:30.5 -- not an asteroid (will add it to exclusion list)
05:55:58.21 +46:42:37.2 -- not an asteroid (will add it to exclusion list)
05:40:02.85 +50:02:04.9 -- not an asteroid (will add it to exclusion list)
06:00:40.09 +44:34:45.4 -- not an asteroid (will add it to exclusion list)
06:01:32.31 +47:32:24.8 -- not an asteroid (will add it to exclusion list)
05:48:46.00 +46:35:02.1 -- not an asteroid (will add it to exclusion list)
05:18:23.05 +45:25:54.9 -- not an asteroid (will add it to exclusion list)
05:48:04.06 +43:19:50.8 -- not an asteroid (will add it to exclusion list)
05:43:52.77 +47:06:14.4 -- not an asteroid (will add it to exclusion list)
05:26:28.90 +41:11:31.1 -- not an asteroid (will add it to exclusion list)
05:28:01.36 +48:15:00.3 -- not an asteroid (will add it to exclusion list)
05:37:46.25 +43:03:12.9 -- not an asteroid (will add it to exclusion list)
05:56:30.92 +46:14:49.3 -- not an asteroid (will add it to exclusion list)
05:25:59.73 +48:30:07.9 -- not an asteroid (will add it to exclusion list)
05:57:46.58 +43:35:10.9 -- not an asteroid (will add it to exclusion list)
05:35:35.23 +44:15:15.1 -- not an asteroid (will add it to exclusion list)
06:01:40.58 +44:57:47.9 -- not an asteroid (will add it to exclusion list)
05:31:00.36 +42:54:52.9 -- not an asteroid (will add it to exclusion list)
06:07:29.92 +46:55:57.3 -- not an asteroid (will add it to exclusion list)
05:27:51.03 +42:20:26.2 -- not an asteroid (will add it to exclusion list)
06:25:49.06 +48:15:44.2 -- not an asteroid (will add it to exclusion list)
06:01:31.69 +42:49:21.1 -- not an asteroid (will add it to exclusion list)
06:02:32.06 +48:11:24.9 -- not an asteroid (will add it to exclusion list)
05:28:11.75 +43:27:55.8 -- not an asteroid (will add it to exclusion list)
05:38:35.64 +41:55:49.6 -- not an asteroid (will add it to exclusion list)
05:27:30.92 +42:33:45.2 -- not an asteroid (will add it to exclusion list)
05:36:14.55 +43:32:31.3 -- not an asteroid (will add it to exclusion list)
05:35:36.13 +47:32:42.8 -- not an asteroid (will add it to exclusion list)
06:46:31.34 +47:39:11.5 -- not an asteroid (will add it to exclusion list)
05:58:13.69 +42:51:14.3 -- not an asteroid (will add it to exclusion list)
06:13:33.57 +48:03:18.1 -- not an asteroid (will add it to exclusion list)
06:15:21.77 +50:34:28.5 -- not an asteroid (will add it to exclusion list)
05:32:56.19 +48:45:35.2 -- not an asteroid (will add it to exclusion list)
05:44:39.82 +43:57:55.7 -- not an asteroid (will add it to exclusion list)
05:53:28.90 +46:52:04.8 -- not an asteroid (will add it to exclusion list)
06:14:39.20 +48:05:36.3 -- not an asteroid (will add it to exclusion list)
05:19:09.74 +44:39:54.1 -- not an asteroid (will add it to exclusion list)
05:39:41.60 +50:57:35.7 -- not an asteroid (will add it to exclusion list)
05:20:50.94 +44:04:37.6 -- not an asteroid (will add it to exclusion list)
05:57:45.39 +45:54:52.3 -- not an asteroid (will add it to exclusion list)
05:40:57.37 +41:07:44.9 -- not an asteroid (will add it to exclusion list)
05:42:50.65 +48:07:39.2 -- not an asteroid (will add it to exclusion list)
05:28:41.38 +48:14:36.0 -- not an asteroid (will add it to exclusion list)
05:37:16.40 +44:02:48.7 -- not an asteroid (will add it to exclusion list)
05:53:51.87 +50:42:48.4 -- not an asteroid (will add it to exclusion list)
06:01:16.81 +47:35:44.8 -- not an asteroid (will add it to exclusion list)
06:23:05.44 +49:11:47.2 -- not an asteroid (will add it to exclusion list)
06:26:29.79 +49:54:10.6 -- not an asteroid (will add it to exclusion list)
05:34:07.90 +42:49:01.2 -- not an asteroid (will add it to exclusion list)
05:48:07.82 +49:40:40.6 -- not an asteroid (will add it to exclusion list)
05:38:36.21 +49:43:22.4 -- not an asteroid (will add it to exclusion list)
05:49:53.28 +45:46:16.6 -- not an asteroid (will add it to exclusion list)
05:57:12.15 +42:33:32.6 -- not an asteroid (will add it to exclusion list)
05:19:05.29 +47:54:37.2 -- not an asteroid (will add it to exclusion list)
05:48:08.81 +44:44:55.2 -- not an asteroid (will add it to exclusion list)
06:04:15.52 +46:54:36.4 -- not an asteroid (will add it to exclusion list)
05:34:19.08 +44:27:44.3 -- not an asteroid (will add it to exclusion list)
05:49:06.52 +47:17:59.3 -- not an asteroid (will add it to exclusion list)
05:42:31.38 +48:39:43.3 -- not an asteroid (will add it to exclusion list)
05:28:27.52 +43:54:02.9 -- not an asteroid (will add it to exclusion list)
05:49:15.68 +45:41:16.2 -- not an asteroid (will add it to exclusion list)
05:52:11.39 +46:15:47.1 -- not an asteroid (will add it to exclusion list)
06:47:02.58 +49:45:30.8 -- not an asteroid (will add it to exclusion list)
05:50:28.74 +44:11:34.7 -- not an asteroid (will add it to exclusion list)
05:56:58.12 +46:41:29.5 -- not an asteroid (will add it to exclusion list)
05:52:58.21 +44:33:09.8 -- not an asteroid (will add it to exclusion list)
05:36:40.74 +50:02:54.9 -- not an asteroid (will add it to exclusion list)
05:45:51.20 +43:22:56.0 -- not an asteroid (will add it to exclusion list)
06:16:06.10 +44:42:54.1 -- not an asteroid (will add it to exclusion list)
05:37:41.41 +45:58:09.0 -- not an asteroid (will add it to exclusion list)
06:07:54.18 +45:58:50.2 -- not an asteroid (will add it to exclusion list)
05:46:44.70 +43:22:54.5 -- not an asteroid (will add it to exclusion list)
05:34:15.91 +44:17:04.7 -- not an asteroid (will add it to exclusion list)
06:36:36.45 +40:24:48.9 -- not an asteroid (will add it to exclusion list)
05:51:25.06 +42:52:21.1 -- not an asteroid (will add it to exclusion list)
06:17:15.78 +49:29:56.5 -- not an asteroid (will add it to exclusion list)
05:39:42.58 +45:03:31.2 -- not an asteroid (will add it to exclusion list)
06:05:14.62 +48:16:56.5 -- not an asteroid (will add it to exclusion list)
06:00:41.06 +40:57:37.3 -- not an asteroid (will add it to exclusion list)
05:41:56.64 +41:07:32.7 -- not an asteroid (will add it to exclusion list)
05:50:48.96 +47:35:39.5 -- not an asteroid (will add it to exclusion list)
05:59:03.69 +45:50:37.0 -- not an asteroid (will add it to exclusion list)
05:54:17.75 +49:03:40.9 -- not an asteroid (will add it to exclusion list)
06:00:34.86 +47:18:29.4 -- not an asteroid (will add it to exclusion list)
06:21:40.27 +49:12:11.0 -- not an asteroid (will add it to exclusion list)
06:06:46.95 +46:38:16.7 -- not an asteroid (will add it to exclusion list)
06:22:49.17 +46:07:41.3 -- not an asteroid (will add it to exclusion list)
05:59:31.97 +48:16:10.6 -- not an asteroid (will add it to exclusion list)
06:41:34.62 +49:47:47.5 -- not an asteroid (will add it to exclusion list)
05:41:47.36 +46:24:57.9 -- not an asteroid (will add it to exclusion list)
05:34:12.98 +50:14:24.7 -- not an asteroid (will add it to exclusion list)
06:01:32.46 +48:06:13.3 -- not an asteroid (will add it to exclusion list)
05:59:14.55 +47:08:48.0 -- not an asteroid (will add it to exclusion list)
06:16:58.55 +49:51:23.5 -- not an asteroid (will add it to exclusion list)
06:01:14.43 +46:27:30.0 -- not an asteroid (will add it to exclusion list)
06:09:09.88 +48:13:10.6 -- not an asteroid (will add it to exclusion list)
05:39:19.04 +50:49:46.9 -- not an asteroid (will add it to exclusion list)
05:34:37.86 +49:13:53.9 -- not an asteroid (will add it to exclusion list)
05:32:33.73 +47:37:16.1 -- not an asteroid (will add it to exclusion list)
05:56:55.23 +47:37:51.6 -- not an asteroid (will add it to exclusion list)
05:45:07.09 +48:23:49.9 -- not an asteroid (will add it to exclusion list)
05:54:54.39 +44:20:23.9 -- not an asteroid (will add it to exclusion list)
06:20:20.72 +45:44:41.6 -- not an asteroid (will add it to exclusion list)
05:22:53.30 +49:01:02.2 -- not an asteroid (will add it to exclusion list)
06:11:23.77 +47:36:13.7 -- not an asteroid (will add it to exclusion list)
05:37:55.68 +43:03:20.1 -- not an asteroid (will add it to exclusion list)
05:51:22.89 +47:46:01.8 -- not an asteroid (will add it to exclusion list)
05:37:17.61 +44:28:41.6 -- not an asteroid (will add it to exclusion list)
05:33:27.70 +48:41:04.7 -- not an asteroid (will add it to exclusion list)
05:53:58.22 +46:34:05.2 -- not an asteroid (will add it to exclusion list)
06:01:52.33 +45:20:53.0 -- not an asteroid (will add it to exclusion list)
05:56:41.19 +46:49:07.2 -- not an asteroid (will add it to exclusion list)
05:46:08.46 +49:03:28.6 -- not an asteroid (will add it to exclusion list)
05:45:22.39 +46:38:00.8 -- not an asteroid (will add it to exclusion list)
05:45:32.61 +50:33:19.1 -- not an asteroid (will add it to exclusion list)
05:40:47.25 +50:52:24.0 -- not an asteroid (will add it to exclusion list)
05:46:07.47 +47:42:00.8 -- not an asteroid (will add it to exclusion list)
05:46:45.05 +46:07:07.8 -- not an asteroid (will add it to exclusion list)
05:55:29.21 +48:34:00.8 -- not an asteroid (will add it to exclusion list)
05:43:36.05 +44:00:57.2 -- not an asteroid (will add it to exclusion list)
06:09:51.91 +46:34:27.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:15:02.20 +48:43:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:54.82 +41:11:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:23.05 +45:25:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:05.29 +47:54:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:09.74 +44:39:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.94 +44:04:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:49.37 +47:17:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:33.99 +48:53:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:53.30 +49:01:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:14.46 +41:03:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.70 +45:40:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:59.73 +48:30:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:28.90 +41:11:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:36.87 +44:48:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:16.19 +45:33:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:18.09 +46:58:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:30.92 +42:33:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:51.03 +42:20:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:01.36 +48:15:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:04.18 +49:28:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:11.75 +43:27:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:27.52 +43:54:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:41.38 +48:14:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:09.72 +43:57:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:00.36 +42:54:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:33.73 +47:37:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:45.81 +42:29:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.19 +48:45:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.89 +44:10:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:27.70 +48:41:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:07.90 +42:49:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:12.98 +50:14:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.91 +44:17:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.08 +44:27:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:37.86 +49:13:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:35.23 +44:15:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:36.13 +47:32:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:47.18 +43:12:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:14.55 +43:32:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.74 +50:02:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.40 +44:02:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:17.61 +44:28:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:22.98 +46:49:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.41 +45:58:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:46.25 +43:03:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:55.68 +43:03:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.34 +41:13:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:35.64 +41:55:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:36.21 +49:43:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.04 +50:49:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:41.60 +50:57:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:42.58 +45:03:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.85 +50:02:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:47.25 +50:52:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:57.37 +41:07:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:47.36 +46:24:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:56.64 +41:07:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:11.17 +44:18:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:31.38 +48:39:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:50.65 +48:07:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:17.36 +42:28:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:36.05 +44:00:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:52.77 +47:06:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:39.82 +43:57:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:07.09 +48:23:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:13.31 +49:30:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:22.39 +46:38:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:32.61 +50:33:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:51.20 +43:22:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:51.96 +50:23:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:07.47 +47:42:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:08.46 +49:03:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:44.70 +43:22:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:45.05 +46:07:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:38.43 +45:18:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.06 +43:19:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:07.82 +49:40:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:08.81 +44:44:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:46.00 +46:35:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.52 +47:17:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:15.68 +45:41:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:47.21 +49:43:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.28 +45:46:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.28 +44:48:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:14.65 +43:23:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.74 +44:11:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:48.96 +47:35:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:22.89 +47:46:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:25.06 +42:52:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:38.20 +48:20:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:55.67 +47:05:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:11.39 +46:15:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:58.21 +44:33:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:23.54 +43:27:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:28.90 +46:52:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:51.87 +50:42:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:58.22 +46:34:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:06.75 +41:46:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:17.75 +49:03:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:54.39 +44:20:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:29.21 +48:34:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:58.21 +46:42:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:09.53 +44:18:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:30.92 +46:14:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:41.19 +46:49:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:48.41 +48:03:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:55.23 +47:37:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:58.12 +46:41:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.15 +42:33:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:45.39 +45:54:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:46.58 +43:35:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:13.69 +42:51:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:03.69 +45:50:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:14.55 +47:08:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:31.97 +48:16:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:34.86 +47:18:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:40.09 +44:34:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:41.06 +40:57:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:13.12 +48:48:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:14.43 +46:27:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.81 +47:35:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:31.69 +42:49:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.31 +47:32:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.46 +48:06:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:40.58 +44:57:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:52.33 +45:20:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.20 +47:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:31.73 +46:29:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.06 +48:11:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.52 +46:54:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:14.62 +48:16:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:28.41 +45:37:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:46.95 +46:38:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:29.92 +46:55:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.18 +45:58:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:09.88 +48:13:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:46.97 +49:06:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.91 +46:34:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:20.87 +50:23:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:13.09 +47:02:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:23.77 +47:36:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:04.60 +50:30:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:25.90 +44:01:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:33.57 +48:03:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:00.15 +49:18:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:39.20 +48:05:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:16.63 +47:16:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:21.77 +50:34:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:06.10 +44:42:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:43.96 +44:42:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:58.55 +49:51:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:15.78 +49:29:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:02.39 +43:28:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:20.72 +45:44:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:40.27 +49:12:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:48.26 +46:46:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:49.17 +46:07:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:05.44 +49:11:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:12.82 +46:48:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:49.06 +48:15:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.79 +49:54:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:36.45 +40:24:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:34.62 +49:47:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.34 +47:39:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:02.58 +49:45:30.8 -- 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)
05:15:02.20 +48:43:56.7 -- not a known variable star
05:17:54.82 +41:11:53.5 -- a known variable star
05:18:23.05 +45:25:54.9 -- not a known variable star
05:19:05.29 +47:54:37.2 -- not a known variable star
05:19:09.74 +44:39:54.1 -- not a known variable star
05:20:50.94 +44:04:37.6 -- not a known variable star
05:21:49.37 +47:17:20.3 -- a known variable star
05:22:33.99 +48:53:35.1 -- a known variable star
05:22:53.30 +49:01:02.2 -- not a known variable star
05:25:14.46 +41:03:21.2 -- a known variable star
05:25:37.70 +45:40:56.7 -- not a known variable star
05:25:59.73 +48:30:07.9 -- not a known variable star
05:26:28.90 +41:11:31.1 -- not a known variable star
05:26:36.87 +44:48:50.0 -- a known variable star
05:27:16.19 +45:33:35.1 -- not a known variable star
05:27:18.09 +46:58:13.2 -- a known variable star
05:27:30.92 +42:33:45.2 -- not a known variable star
05:27:51.03 +42:20:26.2 -- not a known variable star
05:28:01.36 +48:15:00.3 -- a known variable star
05:28:04.18 +49:28:29.4 -- not a known variable star
05:28:11.75 +43:27:55.8 -- not a known variable star
05:28:27.52 +43:54:02.9 -- not a known variable star
05:28:41.38 +48:14:36.0 -- not a known variable star
05:29:09.72 +43:57:13.3 -- not a known variable star
05:31:00.36 +42:54:52.9 -- not a known variable star
05:32:33.73 +47:37:16.1 -- not a known variable star
05:32:45.81 +42:29:58.6 -- not a known variable star
05:32:56.19 +48:45:35.2 -- not a known variable star
05:32:56.89 +44:10:54.0 -- not a known variable star
05:33:27.70 +48:41:04.7 -- not a known variable star
05:34:07.90 +42:49:01.2 -- not a known variable star
05:34:12.98 +50:14:24.7 -- not a known variable star
05:34:15.91 +44:17:04.7 -- not a known variable star
05:34:19.08 +44:27:44.3 -- not a known variable star
05:34:37.86 +49:13:53.9 -- not a known variable star
05:35:35.23 +44:15:15.1 -- not a known variable star
05:35:36.13 +47:32:42.8 -- not a known variable star
05:35:47.18 +43:12:13.9 -- not a known variable star
05:36:14.55 +43:32:31.3 -- not a known variable star
05:36:40.74 +50:02:54.9 -- not a known variable star
05:37:16.40 +44:02:48.7 -- not a known variable star
05:37:17.61 +44:28:41.6 -- a known variable star
05:37:22.98 +46:49:18.4 -- not a known variable star
05:37:41.41 +45:58:09.0 -- not a known variable star
05:37:46.25 +43:03:12.9 -- not a known variable star
05:37:55.68 +43:03:20.1 -- not a known variable star
05:38:27.34 +41:13:51.4 -- not a known variable star
05:38:35.64 +41:55:49.6 -- not a known variable star
05:38:36.21 +49:43:22.4 -- not a known variable star
05:39:19.04 +50:49:46.9 -- not a known variable star
05:39:41.60 +50:57:35.7 -- not a known variable star
05:39:42.58 +45:03:31.2 -- not a known variable star
05:40:02.85 +50:02:04.9 -- not a known variable star
05:40:47.25 +50:52:24.0 -- not a known variable star
05:40:57.37 +41:07:44.9 -- a known variable star
05:41:47.36 +46:24:57.9 -- not a known variable star
05:41:56.64 +41:07:32.7 -- not a known variable star
05:42:11.17 +44:18:00.7 -- a known variable star
05:42:31.38 +48:39:43.3 -- not a known variable star
05:42:50.65 +48:07:39.2 -- not a known variable star
05:43:17.36 +42:28:49.5 -- not a known variable star
05:43:36.05 +44:00:57.2 -- not a known variable star
05:43:52.77 +47:06:14.4 -- not a known variable star
05:44:39.82 +43:57:55.7 -- not a known variable star
05:45:07.09 +48:23:49.9 -- not a known variable star
05:45:13.31 +49:30:40.2 -- not a known variable star
05:45:22.39 +46:38:00.8 -- not a known variable star
05:45:32.61 +50:33:19.1 -- not a known variable star
05:45:51.20 +43:22:56.0 -- a known variable star
05:45:51.96 +50:23:48.3 -- not a known variable star
05:46:07.47 +47:42:00.8 -- not a known variable star
05:46:08.46 +49:03:28.6 -- not a known variable star
05:46:44.70 +43:22:54.5 -- not a known variable star
05:46:45.05 +46:07:07.8 -- not a known variable star
05:47:38.43 +45:18:35.3 -- not a known variable star
05:48:04.06 +43:19:50.8 -- not a known variable star
05:48:07.82 +49:40:40.6 -- not a known variable star
05:48:08.81 +44:44:55.2 -- not a known variable star
05:48:46.00 +46:35:02.1 -- a known variable star
05:49:06.52 +47:17:59.3 -- not a known variable star
05:49:15.68 +45:41:16.2 -- not a known variable star
05:49:47.21 +49:43:02.6 -- a known variable star
05:49:53.28 +45:46:16.6 -- not a known variable star
05:50:10.28 +44:48:35.8 -- not a known variable star
05:50:14.65 +43:23:13.6 -- not a known variable star
05:50:28.74 +44:11:34.7 -- a known variable star
05:50:48.96 +47:35:39.5 -- a known variable star
05:51:22.89 +47:46:01.8 -- not a known variable star
05:51:25.06 +42:52:21.1 -- not a known variable star
05:51:38.20 +48:20:09.2 -- not a known variable star
05:51:55.67 +47:05:43.1 -- a known variable star
05:52:11.39 +46:15:47.1 -- not a known variable star
05:52:58.21 +44:33:09.8 -- a known variable star
05:53:23.54 +43:27:35.3 -- not a known variable star
05:53:28.90 +46:52:04.8 -- not a known variable star
05:53:51.87 +50:42:48.4 -- not a known variable star
05:53:58.22 +46:34:05.2 -- not a known variable star
05:54:06.75 +41:46:11.9 -- a known variable star
05:54:17.75 +49:03:40.9 -- not a known variable star
05:54:54.39 +44:20:23.9 -- not a known variable star
05:55:29.21 +48:34:00.8 -- not a known variable star
05:55:58.21 +46:42:37.2 -- not a known variable star
05:56:09.53 +44:18:00.2 -- not a known variable star
05:56:30.92 +46:14:49.3 -- not a known variable star
05:56:41.19 +46:49:07.2 -- not a known variable star
05:56:48.41 +48:03:55.4 -- not a known variable star
05:56:55.23 +47:37:51.6 -- not a known variable star
05:56:58.12 +46:41:29.5 -- not a known variable star
05:57:12.15 +42:33:32.6 -- not a known variable star
05:57:45.39 +45:54:52.3 -- not a known variable star
05:57:46.58 +43:35:10.9 -- not a known variable star
05:58:13.69 +42:51:14.3 -- not a known variable star
05:59:03.69 +45:50:37.0 -- not a known variable star
05:59:14.55 +47:08:48.0 -- not a known variable star
05:59:31.97 +48:16:10.6 -- not a known variable star
06:00:34.86 +47:18:29.4 -- not a known variable star
06:00:40.09 +44:34:45.4 -- not a known variable star
06:00:41.06 +40:57:37.3 -- not a known variable star
06:01:13.12 +48:48:39.5 -- not a known variable star
06:01:14.43 +46:27:30.0 -- a known variable star
06:01:16.81 +47:35:44.8 -- not a known variable star
06:01:31.69 +42:49:21.1 -- not a known variable star
06:01:32.31 +47:32:24.8 -- not a known variable star
06:01:32.46 +48:06:13.3 -- not a known variable star
06:01:40.58 +44:57:47.9 -- not a known variable star
06:01:52.33 +45:20:53.0 -- not a known variable star
06:02:14.20 +47:47:00.4 -- a known variable star
06:02:31.73 +46:29:05.7 -- not a known variable star
06:02:32.06 +48:11:24.9 -- not a known variable star
06:04:15.52 +46:54:36.4 -- not a known variable star
06:05:14.62 +48:16:56.5 -- not a known variable star
06:05:28.41 +45:37:48.9 -- not a known variable star
06:06:46.95 +46:38:16.7 -- not a known variable star
06:07:29.92 +46:55:57.3 -- not a known variable star
06:07:54.18 +45:58:50.2 -- not a known variable star
06:09:09.88 +48:13:10.6 -- not a known variable star
06:09:46.97 +49:06:39.5 -- not a known variable star
06:09:51.91 +46:34:27.5 -- a known variable star
06:10:20.87 +50:23:13.5 -- not a known variable star
06:11:13.09 +47:02:39.1 -- not a known variable star
06:11:23.77 +47:36:13.7 -- not a known variable star
06:12:04.60 +50:30:17.1 -- not a known variable star
06:13:25.90 +44:01:20.9 -- a known variable star
06:13:33.57 +48:03:18.1 -- not a known variable star
06:14:00.15 +49:18:13.1 -- not a known variable star
06:14:39.20 +48:05:36.3 -- not a known variable star
06:15:16.63 +47:16:52.4 -- not a known variable star
06:15:21.77 +50:34:28.5 -- not a known variable star
06:16:06.10 +44:42:54.1 -- not a known variable star
06:16:43.96 +44:42:41.2 -- not a known variable star
06:16:58.55 +49:51:23.5 -- not a known variable star
06:17:15.78 +49:29:56.5 -- not a known variable star
06:18:02.39 +43:28:06.6 -- not a known variable star
06:20:20.72 +45:44:41.6 -- not a known variable star
06:21:40.27 +49:12:11.0 -- a known variable star
06:21:48.26 +46:46:30.5 -- not a known variable star
06:22:49.17 +46:07:41.3 -- not a known variable star
06:23:05.44 +49:11:47.2 -- not a known variable star
06:23:12.82 +46:48:44.6 -- not a known variable star
06:25:49.06 +48:15:44.2 -- not a known variable star
06:26:29.79 +49:54:10.6 -- not a known variable star
06:36:36.45 +40:24:48.9 -- not a known variable star
06:41:34.62 +49:47:47.5 -- not a known variable star
06:46:31.34 +47:39:11.5 -- not a known variable star
06:47:02.58 +49:45:30.8 -- not a known variable star
Found 142 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
165 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 165 (excluding asteroids and hot pixels, 142 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)2461147.66183569 -observatory V36
00:13:29.31 -01:24:20.1 Mercury (0.0mag)
03:14:20.32 +18:17:16.4 Venus (-3.9mag)
00:21:08.39 +01:13:39.2 Mars (1.2mag)
07:13:09.93 +22:45:21.0 Jupiter (-2.1mag)
00:29:41.86 +00:52:11.9 Saturn (0.9mag)
03:47:56.56 +19:48:15.8 Uranus (5.8mag)
00:10:59.49 -00:14:25.1 Neptune (7.8mag)
20:33:48.24 -22:52:39.3 Pluto (14.5mag)
01:14:33.85 +11:20:18.3 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Apr 16 23:00 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461147.66183569:
07:13:05.00 +22:45:29.1 Io (5.8mag)
07:13:19.78 +22:44:57.9 Europa (5.9mag)
07:13:11.97 +22:45:09.4 Ganymede (5.4mag)
07:13:42.85 +22:44:09.7 Callisto (6.6mag)
07:16:27.06 +22:32:26.5 Himalia (15.3mag)
07:13:13.30 +22:45:14.9 Thebe (16.2mag)
07:16:39.92 +23:02:42.2 Elara (17.3mag)
07:12:07.56 +23:24:44.9 Pasiphae (17.4mag)
07:21:28.07 +22:43:29.0 Carme (18.5mag)
00:29:38.28 +00:52:39.7 Titan (8.8mag)
00:29:46.47 +00:52:10.9 Rhea (10.1mag)
00:29:19.98 +00:52:10.1 Iapetus (11.5mag)
00:29:45.85 +00:52:36.6 Hyperion (14.8mag)
00:31:17.83 +01:00:52.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 16 23:00 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461147.66183569:
15:43:29.93 -17:03:24.5 JWST
17:41:23.56 +38:22:09.3 Chandra
17:21:45.11 -47:22:44.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 16 23:00 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461147.66183569 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:27.65 -28:50:51.8 13.9mag P/2010 H2 (Vales)
05:07:34.58 -69:36:26.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:42.09 +31:26:43.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:18.78 +10:41:04.9 17.6mag C/2021 G2 (ATLAS)
23:10:31.62 +29:16:31.6 17.1mag C/2022 E2 (ATLAS)
04:30:35.59 +26:04:11.0 16.0mag C/2022 N2 (PANSTARRS)
09:03:40.86 +32:01:24.7 16.2mag C/2022 QE78 (ATLAS)
08:31:15.62 -00:01:52.2 17.3mag C/2022 R6 (PANSTARRS)
18:53:26.75 +18:37:46.1 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:17.54 -11:30:16.3 17.5mag P/2023 B1 (PANSTARRS)
09:07:06.71 -11:41:54.3 17.6mag C/2023 F3 (ATLAS)
21:55:21.70 +62:58:30.6 17.5mag C/2023 H5 (Lemmon)
19:18:10.03 -03:45:09.3 14.1mag C/2023 R1 (PANSTARRS)
21:29:56.80 +86:04:23.7 17.8mag C/2023 X2 (Lemmon)
06:18:27.72 +63:30:30.5 17.2mag C/2024 A1 (ATLAS)
05:15:44.83 +18:41:10.6 11.1mag C/2024 E1 (Wierzchos)
16:18:31.21 +06:34:50.0 17.4mag C/2024 G6 (ATLAS)
20:21:07.52 +15:35:29.1 14.6mag C/2024 J3 (ATLAS)
03:27:24.95 -22:12:35.0 16.3mag C/2024 T5 (ATLAS)
05:17:42.20 +45:00:18.1 17.7mag C/2025 J1 (Borisov)
13:34:01.57 +46:12:59.7 15.2mag C/2025 L1 (ATLAS)
03:27:07.46 -26:23:41.0 17.8mag C/2025 Q3 (ATLAS)
23:54:37.04 +18:08:52.0 8.3mag C/2025 R3 (PANSTARRS)
12:53:37.05 +03:04:57.6 17.4mag C/2025 Y1 (ATLAS)
03:37:04.71 +02:30:13.0 13.6mag C/2026 A1 (MAPS)
00:02:51.22 +37:25:47.3 14.6mag C/2026 B2 (Sun-Gao)
18:45:11.79 -09:39:23.2 11.8mag 10P/Tempel
14:58:43.70 +03:05:08.6 14.1mag 24P/Schaumasse
11:02:30.03 -01:29:21.5 15.7mag 29P/Schwassmann-Wachmann
18:01:16.14 -09:34:05.3 18.0mag 40P/Vaisala
10:37:32.28 -04:00:30.5 16.9mag 43P/Wolf-Harrington
01:50:28.37 +17:41:06.2 17.2mag 47P/Ashbrook-Jackson
07:12:55.30 +36:45:44.1 17.0mag 63P/Wild
23:30:31.97 -11:18:43.1 15.7mag 65P/Gunn
04:06:22.09 +21:39:02.5 15.9mag 76P/West-Kohoutek-Ikemura
01:08:08.88 +08:27:23.2 14.3mag 78P/Gehrels
23:06:30.22 -09:02:50.4 14.6mag 88P/Howell
02:13:42.04 +20:56:59.4 15.1mag 93P/Lovas
04:57:00.43 +32:20:55.5 16.2mag 123P/West-Hartley
08:29:45.16 +37:49:32.1 16.2mag 124P/Mrkos
02:35:00.88 +14:29:56.5 16.4mag 128P/Shoemaker-Holt
02:49:49.13 +14:38:01.5 17.5mag 131P/Mueller
01:32:17.68 +13:37:58.8 10.6mag 141P/Machholz
01:41:03.24 +05:18:31.5 10.6mag 141P-A/Machholz
00:25:48.47 +01:10:44.4 12.7mag 141P-D/Machholz
02:11:28.09 +07:04:06.4 17.8mag 141P-I/Machholz
01:05:37.36 -00:56:25.8 15.1mag 162P/SidingSpring
14:49:22.44 +00:02:54.8 17.7mag 210P/Christensen
21:42:10.35 -11:10:09.0 17.6mag 218P/LINEAR
17:16:49.55 -13:47:34.2 16.1mag 235P/LINEAR
05:36:59.93 +34:47:04.4 16.8mag 240P/NEAT
07:39:04.58 -05:02:34.4 17.7mag 242P/Spahr
22:19:48.81 -20:40:04.2 17.9mag 260P/McNaught
02:00:34.00 +20:45:06.8 18.0mag 295P/LINEAR
15:42:10.98 +07:03:57.8 17.5mag 391P/Kowalski
07:34:39.19 +21:22:08.7 17.7mag 450P/LONEOS
05:37:34.42 +44:57:53.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 16 23:00 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
-rw-r--r-- 1 apache apache 5.8K Apr 16 23:00 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 16 23:00 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:06:56.603 -64:55:52.46 AT 2026jcy 2026-04-09.11 18.906
08:27:06.222 -58:50:26.83 AT 2026jcx 2026-04-09.08 19.372
13:48:22.893 -31:10:42.12 AT 2026jcw 2026-04-09.08 19.95
17:39:28.750 +05:01:10.80 AT 2026jcv 2026-04-09.86 16.87
14:44:31.580 +71:55:25.90 AT 2026jcu 2026-04-09.47 17.9
12:39:27.288 -08:14:32.64 AT 2026jct 2026-04-09.53 20.16
14:15:21.948 -35:02:48.79 AT 2026jcs 2026-04-09.59 19.67
12:55:53.000 +08:04:22.00 AT 2026jcr 2026-04-09.62 22.1051
12:29:42.630 -28:00:38.18 AT 2026jcq 2026-04-09.56 18.99
13:00:14.826 -06:35:50.60 AT 2026jcp 2026-04-09.56 19.7
12:54:45.376 +09:10:41.41 AT 2026jco 2026-04-09.62 20.9256
13:25:12.570 -33:30:18.80 AT 2026jcn 2026-04-07.60 19.74
13:20:52.501 -35:57:03.67 AT 2026jcm 2026-04-07.60 20.01
12:07:08.367 +13:12:39.86 AT 2026jcl 2026-04-09.62 22.8073
12:11:43.063 +14:00:46.62 AT 2026jck 2026-04-09.62 21.8834
14:57:35.040 -17:11:22.89 AT 2026jcj 2026-04-09.58 19.52
15:09:26.181 -10:41:27.18 AT 2026jci 2026-04-09.45 20.2
18:22:34.467 +53:35:59.16 AT 2026jch 2026-04-05.40 19.7444
15:13:25.280 +39:43:46.60 AT 2026jcg 2026-03-30.81 21.1
17:32:02.830 +27:34:31.03 AT 2026jcf 2026-03-27.92 21.46
-rw-r--r-- 1 apache apache 30K Apr 16 23:00 tns_transients_list.txt
