This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae
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
AC Aur,2461149.6588,11.34,0.05,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
AC Aur 20260419.1588 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209684259058288384,2461149.6588,13.96,0.05,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 209684259058288384 20260419.1588 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3354+46.2593,2461149.6588,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.3354+46.2593 20260419.1588 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.83,0.05,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 20260419.1588 13.83CV 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
ATO J087.5522+44.8128,2461149.6588,13.64,0.05,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 J087.5522+44.8128 20260419.1588 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
ASASSN-V J055127.94+451129.9,2461149.6588,13.61,0.05,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
ASASSN-V J055127.94+451129.9 20260419.1588 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1932+42.5719,2461149.6588,13.68,0.05,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 J084.1932+42.5719 20260419.1588 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2887+47.4652,2461149.6588,13.82,0.05,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
ATO J089.2887+47.4652 20260419.1588 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,2461149.6588,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3686+43.2939,2461149.6588,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3686+43.2939 20260419.1588 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.40,0.05,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
target 20260419.1588 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 196107828779642752,2461149.6588,13.37,0.05,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
Gaia DR3 196107828779642752 20260419.1588 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967581128777104000,2461149.6588,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967581128777104000 20260419.1588 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6295+48.7004,2461149.6588,13.31,0.05,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 J084.6295+48.7004 20260419.1588 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 J085.1267+46.2073,2461149.6588,13.12,0.05,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 J085.1267+46.2073 20260419.1588 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196183179687428352,2461149.6588,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196183179687428352 20260419.1588 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 J089.2781+45.3867,2461149.6588,13.04,0.05,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 J089.2781+45.3867 20260419.1588 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060214.12+474700.6,2461149.6588,13.21,0.05,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
ASASSN-V J060214.12+474700.6 20260419.1588 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.1833+42.4993,2461149.6588,12.86,0.05,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 J083.1833+42.4993 20260419.1588 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,12.59,0.05,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 20260419.1588 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,12.43,0.05,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 20260419.1588 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 962371397869379840,2461149.6588,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962371397869379840 20260419.1588 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.8851+48.3378,2461149.6588,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.8851+48.3378 20260419.1588 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192332281946145280,2461149.6588,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192332281946145280 20260419.1588 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968399680823767936,2461149.6588,9.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968399680823767936 20260419.1588 9.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3456+46.8139,2461149.6588,10.16,0.05,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 J084.3456+46.8139 20260419.1588 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193611559426097664,2461149.6588,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193611559426097664 20260419.1588 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208934456550670592,2461149.6588,11.22,0.05,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 20260419.1588 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
ATO J085.0114+50.0334,2461149.6588,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.0114+50.0334 20260419.1588 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208736750615473024,2461149.6588,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208736750615473024 20260419.1588 11.97CV 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 J087.0101+43.3293,2461149.6588,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.0101+43.3293 20260419.1588 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963045020540085504,2461149.6588,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963045020540085504 20260419.1588 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.3861+47.5396,2461149.6588,12.44,0.05,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 J090.3861+47.5396 20260419.1588 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,2461149.6588,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 J091.9030+46.9269,2461149.6588,12.68,0.05,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 J091.9030+46.9269 20260419.1588 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 J089.2046+48.9230,2461149.6588,12.64,0.05,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 J089.2046+48.9230 20260419.1588 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209019462542689536,2461149.6588,12.46,0.05,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 209019462542689536 20260419.1588 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 J092.0097+46.6828,2461149.6588,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.0097+46.6828 20260419.1588 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.0658+43.5403,2461149.6588,12.65,0.05,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
ATO J084.0658+43.5403 20260419.1588 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 J082.7523+42.9146,2461149.6588,12.64,0.05,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 J082.7523+42.9146 20260419.1588 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 J083.6752+47.3369,2461149.6588,12.62,0.05,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 J083.6752+47.3369 20260419.1588 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461149.6588,12.81,0.05,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
Gaia DR3 211485843219678720 20260419.1588 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461149.6588,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.6351+48.1884 20260419.1588 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.8963+44.2568,2461149.6588,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8963+44.2568 20260419.1588 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.9230+50.9576,2461149.6588,12.80,0.05,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 J084.9230+50.9576 20260419.1588 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,2461149.6588,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 J087.2715+41.2989,2461149.6588,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2715+41.2989 20260419.1588 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968792687512124800,2461149.6588,12.95,0.05,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
Gaia DR3 968792687512124800 20260419.1588 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.2234+48.7629,2461149.6588,12.81,0.05,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 J083.2234+48.7629 20260419.1588 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
Gaia DR3 208940641302877696,2461149.6588,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208940641302877696 20260419.1588 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.9773+46.5565,2461149.6588,13.04,0.05,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 J081.9773+46.5565 20260419.1588 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 J093.3774+41.9686,2461149.6588,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3774+41.9686 20260419.1588 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7835+47.9155,2461149.6588,12.95,0.05,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 J079.7835+47.9155 20260419.1588 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 197388553666998656,2461149.6588,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197388553666998656 20260419.1588 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 970672714956491008,2461149.6588,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970672714956491008 20260419.1588 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461149.6588,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5805+44.4532 20260419.1588 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.14,0.05,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
target 20260419.1588 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.6786+45.4850,2461149.6588,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.6786+45.4850 20260419.1588 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 J090.6026+48.3315,2461149.6588,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.6026+48.3315 20260419.1588 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 J083.5567+44.2856,2461149.6588,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5567+44.2856 20260419.1588 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 213847422398656512,2461149.6588,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 213847422398656512 20260419.1588 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970027988825374592,2461149.6588,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970027988825374592 20260419.1588 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461149.6588,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2776+47.3006 20260419.1588 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 J087.2220+45.5909,2461149.6588,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2220+45.5909 20260419.1588 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6873+48.2843,2461149.6588,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.6873+48.2843 20260419.1588 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.14,0.05,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
target 20260419.1588 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461149.6588,13.32,0.05,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
ATO J084.1629+50.0440 20260419.1588 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
ATO J084.7951+42.7560,2461149.6588,13.41,0.05,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 J084.7951+42.7560 20260419.1588 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
ASASSN-V J053745.20+455814.5,2461149.6588,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J053745.20+455814.5 20260419.1588 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 J089.5381+48.6224,2461149.6588,13.31,0.05,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 J089.5381+48.6224 20260419.1588 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212237526922373120,2461149.6588,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212237526922373120 20260419.1588 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963318524057490944,2461149.6588,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963318524057490944 20260419.1588 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963235824465355264,2461149.6588,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963235824465355264 20260419.1588 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.6953+44.0131,2461149.6588,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.6953+44.0131 20260419.1588 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2615+46.3117,2461149.6588,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.2615+46.3117 20260419.1588 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.3958+50.3918,2461149.6588,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.3958+50.3918 20260419.1588 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 J093.1689+45.0683,2461149.6588,13.65,0.05,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 J093.1689+45.0683 20260419.1588 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 J084.4519+43.0341,2461149.6588,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.4519+43.0341 20260419.1588 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 19.1588 2461149.6588 13.66 05:44:09.94 +51:12:01.5
160.62384 11.18727 galactic Aur Second-epoch detections are separated by 2.8" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 215231157781140608 | 05:44:09.94 +51:12:01.5 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.013+/-0.082 (M)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 215231157781140608,2461149.6588,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 215231157781140608 20260419.1588 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210216624548997760,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210216624548997760 20260419.1588 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2458+42.7482,2461149.6588,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.2458+42.7482 20260419.1588 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 J089.6159+43.7708,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.6159+43.7708 20260419.1588 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 208475208586436992,2461149.6588,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208475208586436992 20260419.1588 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209295547338780928,2461149.6588,13.65,0.05,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 209295547338780928 20260419.1588 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 209760572037087744,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209760572037087744 20260419.1588 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.9114+46.7779,2461149.6588,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.9114+46.7779 20260419.1588 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.65,0.05,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
target 20260419.1588 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.99,0.05,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
target 20260419.1588 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.4195+46.7700,2461149.6588,13.68,0.05,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 J085.4195+46.7700 20260419.1588 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 212069267283233408,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 212069267283233408 20260419.1588 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
target,2461149.6588,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.6230+40.9605,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.6230+40.9605 20260419.1588 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
target,2461149.6588,13.78,0.05,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 20260419.1588 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
target,2461149.6588,13.72,0.05,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 20260419.1588 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967755573168122368,2461149.6588,13.92,0.05,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 967755573168122368 20260419.1588 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 967694309755022976,2461149.6588,13.74,0.05,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 967694309755022976 20260419.1588 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.5843+47.3818,2461149.6588,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.5843+47.3818 20260419.1588 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.81,0.05,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
target 20260419.1588 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
target,2461149.6588,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.7435+47.6163,2461149.6588,13.65,0.05,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 J082.7435+47.6163 20260419.1588 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5355+49.9005,2461149.6588,13.81,0.05,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 J089.5355+49.9005 20260419.1588 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 968357899382262912,2461149.6588,13.81,0.05,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 968357899382262912 20260419.1588 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 J082.6857+49.0456,2461149.6588,13.73,0.05,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 J082.6857+49.0456 20260419.1588 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 J084.2481+47.3417,2461149.6588,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.2481+47.3417 20260419.1588 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.96,0.05,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 20260419.1588 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.95,0.05,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 20260419.1588 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
ATO J087.7045+40.9462,2461149.6588,13.82,0.05,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
ATO J087.7045+40.9462 20260419.1588 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,2461149.6588,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.81,0.05,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
target 20260419.1588 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 J081.1447+48.2716,2461149.6588,13.78,0.05,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
ATO J081.1447+48.2716 20260419.1588 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
target,2461149.6588,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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 J092.2022+47.5751,2461149.6588,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.2022+47.5751 20260419.1588 13.92CV 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 J089.1139+42.7270,2461149.6588,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1139+42.7270 20260419.1588 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.1119+47.8573,2461149.6588,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.1119+47.8573 20260419.1588 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209594442702454912,2461149.6588,13.88,0.05,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 209594442702454912 20260419.1588 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
target,2461149.6588,13.72,0.05,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 20260419.1588 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.79,0.05,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
target 20260419.1588 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 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
target,2461149.6588,13.96,0.05,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 20260419.1588 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.5570+43.7626,2461149.6588,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J082.5570+43.7626 20260419.1588 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1588 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 969737610380466176,2461149.6588,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 969737610380466176 20260419.1588 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6588,13.99,0.05,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
target 20260419.1588 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.1131+41.5636,2461149.6588,13.77,0.05,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
ATO J087.1131+41.5636 20260419.1588 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,2461149.6588,13.95,0.05,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 20260419.1588 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
Gaia DR3 214349212017034496,2461149.6588,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 214349212017034496 20260419.1588 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.3197+46.8663,2461149.6588,13.95,0.05,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
ATO J085.3197+46.8663 20260419.1588 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
VY Aur,2461149.6588,11.49,0.05,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 20260419.1588 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: 2461149.65915507 19.04.2026 03:49:00.998 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
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: 8 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23194
Objects passed selection criteria: 23173
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 21080.5
Average stars matched: 20610.5 (97.7705 %)
Memory usage VmPeak: 126880 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 22:53:07 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: 2461149.65915507 19.04.2026 03:49:00.998 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 612
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: 133 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): 166903
Objects passed selection criteria: 166521
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: 157773
Average stars matched: 152479 (96.6447 %)
Memory usage VmPeak: 1982076 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 22:57:26 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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461149.65853236
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits'
wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Image size: 941.7'x626.7' 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: 06:00:19.247 +45:58:06.82 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 06:00:19.247 +45:58:06.82
Angular distance between the image centers 0.0999 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Image size: 941.7'x626.7' 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: 06:00:19.619 +45:58:08.19 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 06:00:19.619 +45:58:08.19
Angular distance between the image centers 0.1007 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 06:00:19.247 +45:58:06.82
Second-epoch second image center 06:00:19.619 +45:58:08.19
Angular distance between the image centers 0.00114 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00114 deg. (min. required shift: 0.00164 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.U3KU277eqL
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.JyrFrVoLeO
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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits &> /tmp/tmp.Hb5ONDg0yc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits &> /tmp/tmp.UU6GoZjWfF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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 19 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
2.1 pix fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
2.1 pix fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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
15.1 mag. fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
15.1 mag. fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (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.U3KU277eqL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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.JyrFrVoLeO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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.Hb5ONDg0yc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1418, passed=18149
Got 18149 stars (including 16695 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat
util/solve_plate_with_UCAC5 got 18149 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 913 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(), 17579 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 934 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(), 17580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 17580 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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.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.UU6GoZjWfF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1397, passed=18132
Got 18132 stars (including 16704 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat
util/solve_plate_with_UCAC5 got 18132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 17655 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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 17654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 17654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits'
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02325.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31503_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31503_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:36:22.14 +47:50:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31547_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31547_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:27.47 +44:52:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)GAIADR2_OUTPUT=# 1.127 207908784002418688 083.61485843374 +44.87196594922 10.2491 9.4244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31553_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31553_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:14:59.10 +46:47:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31575_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31575_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:59:43.43 +44:59:10.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 31587_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31587_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:28.49 +43:00:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31589_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31589_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:23.03 +46:49:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.561 209803315551351552 084.34589502799 +46.82176702889 11.3001 10.9865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31650_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31650_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:45:42.88 +43:37:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31690_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31690_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:21.20 +50:18:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31697_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31697_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:11:34.44 +48:44:36.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31699_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31699_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:17.88 +45:35:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31713_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31713_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:47:38.69 +48:43:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.574 990868338376216576 101.91139967351 +48.72968045974 12.1359 11.6220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31716_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31716_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 31719_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31719_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:09:52.00 +46:34:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.949 963406141390333184 092.46702943046 +46.57449767313 10.4625 8.8819 VARIABLE#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 31727_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31727_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 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=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)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 31736_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31736_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:23.85 +48:22:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31746_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 31746_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:02:56.18 +45:31:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.663 963139406741412736 090.73430592721 +45.52917993704 12.3198 11.8472 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13041_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 13041_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 02325_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00905_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 00905_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:01.76 +50:29:26.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field 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 ####
05:27:04.81 +50:07:24.0
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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits exists and is non-empty
wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Image size: 941.7'x626.7' 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: 06:00:19.247 +45:58:06.82 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 06:00:19.247 +45:58:06.82
Angular distance between the image centers 0.0999 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Image size: 941.7'x626.7' 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: 06:00:19.619 +45:58:08.19 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 06:00:19.619 +45:58:08.19
Angular distance between the image centers 0.1007 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 06:00:19.247 +45:58:06.82
Second-epoch second image center 06:00:19.619 +45:58:08.19
Angular distance between the image centers 0.00114 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00114 deg. (min. required shift: 0.00164 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.yHNieWScuv
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.v6HTEXjMD7
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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits &> /tmp/tmp.if2F9e2nwx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits &> /tmp/tmp.OEaRXW9IpL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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 576 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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
2.0 pix fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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
14.2 mag. fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
14.2 mag. fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (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.yHNieWScuv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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.v6HTEXjMD7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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.if2F9e2nwx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=13490, passed=147446
Got 147446 stars (including 133692 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat
util/solve_plate_with_UCAC5 got 147446 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 145001 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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 145002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 145003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.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.OEaRXW9IpL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Checking if the catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat corresponding to the image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
WCS catalog name: wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=13318, passed=146484
Got 146484 stars (including 132915 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat
util/solve_plate_with_UCAC5 got 146484 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 936 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 144145 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 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 144144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 144144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits -region wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/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_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-48-07_20.00sec_-4.90C_LIGHTs_0307.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-02-Q1b1x1_224951_TTUQ1b1x1_2253989_sRiFLIae/wcs_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308.fits
Preparing the HTML report for the field Aur-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out195247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out195253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197111.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__out197131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198088.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): 235s
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: 100s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195247_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195247_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:31:13.64 +49:04:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.198 212761792104487936 082.80683163961 +49.08311159775 14.4174 13.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195254_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195254_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195258_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195258_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:41.07 +49:33:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.405 214244620973660032 084.42156877971 +49.56662458220 14.7575 14.0186 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195273_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195273_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195279_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195279_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:13:59.82 +49:18:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.130 969387351503471104 093.49968336657 +49.30775203185 14.4278 13.9576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195281_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195285_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195285_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195286_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195286_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195295_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195295_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195300_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195300_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195303_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195303_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:45:10.26 +42:25:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.665 192981165604050304 086.29336500635 +42.42338390233 14.2650 13.4757 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195307_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195307_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195309_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195309_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:50:38.31 +46:28:16.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 195313_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195313_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:49.25 +48:57:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.433 214015750756237440 083.70511604589 +48.96077313812 14.5731 13.7425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195314_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195314_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:18:41.62 +42:18:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195316_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195316_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:55:49.03 +44:04:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.129 193593696660200320 088.95437621220 +44.07180341739 14.7013 14.1169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195318_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195318_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195322_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195322_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:24.48 +44:48:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.747 197387492812802688 084.35309392447 +44.80025087634 14.4821 13.6422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195342_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195342_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:24.47 +50:20:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.135 211569852780732288 089.35236411573 +50.33418129791 14.5141 13.8996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195346_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195346_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:20:01.48 +42:43:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.833 207310757053355008 080.00629222866 +42.72755485151 14.0499 13.1689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195347_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195347_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195349_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195349_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:36.41 +48:19:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195354_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195354_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:50:29.13 +50:48:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.181 214608142708363904 087.62182050965 +50.80269248900 14.4520 13.7482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195357_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195357_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:27.38 +43:48:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.090 195611163059241088 083.61450272044 +43.80372310162 14.1797 13.5453 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 195361_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195361_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195363_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195363_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195364_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195364_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:18:54.00 +41:36:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195366_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195366_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:35:18.39 +41:12:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.375 194361361935740160 083.82693520335 +41.20125325123 14.2482 13.6927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195369_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195369_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:09:13.86 +41:30:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195370_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195370_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195372_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195372_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195373_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195373_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:34.69 +45:49:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.515 209499815983191808 084.64501969201 +45.82343726759 14.0922 13.0991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195376_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195376_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:20.15 +41:55:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.455 193092800394897280 087.33390194821 +41.92263064796 14.2183 13.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195377_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195377_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:59.39 +49:26:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.544 211286694176443648 089.24755543055 +49.44861273434 14.4035 13.8229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195381_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195381_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:20:28.40 +41:32:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.821 194914244485852160 080.11832344052 +41.54446653863 14.0776 13.1443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195382_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195384_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195384_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:42:47.75 +50:23:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.887 214377043404958464 085.69887447197 +50.38382386812 14.4119 13.6273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195385_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195385_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:54.81 +47:08:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.024 211944683168243328 080.47915916318 +47.13573326299 14.3664 13.5179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195388_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195388_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195394_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195395_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195400_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195401_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195401_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:57.64 +42:35:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195409_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195409_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:35:12.68 +44:57:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.148 207915351008628736 083.80326574230 +44.96346521822 14.3639 13.7945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195412_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195418_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195418_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:04:16.55 +44:03:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195424_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195424_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:21.29 +41:17:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195426_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195426_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:29.34 +50:53:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.365 213907242702848896 082.62243045009 +50.88366608650 14.1676 13.6215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195427_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195428_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195428_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:29:51.86 +50:44:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195430_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195430_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:35:00.14 +50:18:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195434_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195434_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:44.44 +50:48:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195435_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195435_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:31.19 +42:08:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.625 195038111342984832 081.38049763012 +42.14459603839 14.0228 13.5076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195439_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195439_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:15:23.44 +51:00:02.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 195451_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195451_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:37:57.22 +48:39:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.798 967727363823117952 099.48862716078 +48.65527176913 14.3365 13.6999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195454_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195454_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195455_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195455_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195458_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195458_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:05:39.41 +42:41:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195459_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195459_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:35:51.54 +48:37:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.925 967736537873159552 098.96442617276 +48.62908682184 13.9840 13.4169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195460_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195460_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:50:24.52 +47:19:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.545 210015452576247680 087.60279277924 +47.33165814040 14.0999 13.2662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195461_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195461_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195462_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195462_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:48.84 +43:07:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195468_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195471_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195471_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195482_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195482_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:37.78 +42:12:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195483_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195498_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195498_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:46.42 +48:52:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195502_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195502_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:59.63 +44:37:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.872 207708127426423808 080.74876747824 +44.62546209328 13.6319 12.8108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195503_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195503_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:15.47 +43:36:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195505_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195505_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:15:57.55 +41:11:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195507_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195507_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:59.27 +46:26:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.428 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195510_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195510_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195512_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195512_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:31:27.63 +47:36:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195514_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195514_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195521_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195521_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:18:32.78 +46:16:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.770 211837721303196800 079.63671201134 +46.28305578216 13.5567 13.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195525_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195525_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195527_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195527_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:32.35 +41:33:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.445 194386856861482496 083.63319066159 +41.56110461880 13.5151 12.6425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195528_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195528_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:53.47 +43:56:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195531_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195531_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:50.71 +41:27:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195535_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195535_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:53.67 +50:04:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195537_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195537_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:36:55.59 +50:56:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195539_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195539_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195540_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195540_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:19.51 +45:53:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.900 208774413187367296 080.33164408935 +45.88731042565 13.5455 12.9311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195542_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195542_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:47.34 +42:06:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195548_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195548_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:00.05 +43:23:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195549_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195549_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:24.61 +42:28:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195551_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195551_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:31:36.57 +45:36:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195552_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195552_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195557_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195557_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:11:13.09 +47:02:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.836 969416385483084800 092.80474694837 +47.04423121691 13.2454 12.7727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195560_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195560_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:31:06.75 +48:10:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195563_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195563_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:47.71 +43:12:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195566_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195566_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:37.08 +41:20:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195567_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195567_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:40:23.55 +49:53:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195569_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195569_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195570_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195570_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:28:28.82 +48:44:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195572_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195572_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195574_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195574_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:54:42.21 +43:39:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.485 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195577_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195577_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:45.95 +43:34:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195579_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195579_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:09.03 +46:13:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 0.753 197771561669756288 089.28789413872 +46.22871042011 12.0773 11.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195580_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195580_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:26:48.20 +43:44:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195582_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195582_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195656_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195656_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:43:27.54 +42:19:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.19, MAG_FAINT_SEARCH_LIMIT=11.17)GAIADR2_OUTPUT=# 0.305 193022397288096512 085.86480449930 +42.32350876868 10.9773 10.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195663_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195663_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:28.50 +43:00:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195667_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195667_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:28.75 +50:02:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195668_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195668_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:44:52.58 +49:21:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195669_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195669_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195670_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195670_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:08:02.88 +48:43:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195698_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195698_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195731_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195731_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:45:42.88 +43:37:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195743_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195743_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195748_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195748_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195761_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195761_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195782_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195782_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:11:34.51 +48:44:35.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195795_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195795_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:58:32.68 +44:49:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195799_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195799_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195802_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195802_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195805_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195805_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195809_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195809_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:32.52 +43:37:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195819_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195819_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195844_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195844_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:43:31.43 +50:41:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 0.248 214454073641026304 085.88098036325 +50.69193240962 12.2176 11.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195846_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195846_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195851_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195851_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:01.48 +41:06:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195864_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195864_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:46:26.57 +47:55:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 1.106 209974903788049920 086.61100294443 +47.91704234689 12.4908 11.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195872_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195872_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:33:38.39 +45:26:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195878_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195878_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195881_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195881_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195883_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195883_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:26:36.53 +40:59:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195890_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195890_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:06:21.40 +48:46:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 1.053 969866223177226368 091.58945434374 +48.77666602788 12.4108 11.4977 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195911_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195911_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195923_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195923_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:17.72 +45:03:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195935_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195935_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195953_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195953_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:09.76 +47:19:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.566 212316245079377280 081.04053074053 +47.31751152611 12.7573 12.0006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195961_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195961_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195963_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195963_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195966_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195966_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195975_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195975_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195981_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 195981_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 195986_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195986_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:37.59 +45:55:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195988_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195988_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:39:07.57 +44:53:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.951 197368109622667392 084.78191388712 +44.88670652218 12.6990 11.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195997_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195997_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 195999_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 195999_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196007_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196007_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:51.88 +42:57:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196017_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196017_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:48.32 +46:57:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.979 198029362786762880 089.20161100133 +46.96494369065 12.8922 12.0517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196037_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196037_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:18:23.56 +48:55:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196042_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196042_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196043_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196043_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196054_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196054_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196057_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196057_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:05:50.21 +44:39:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.543 962961320218080000 091.45935160151 +44.65874992474 12.7976 12.0911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196059_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196059_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196060_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196060_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196064_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196064_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:40.84 +44:01:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.184 207441461497335040 081.17062388152 +44.02989922297 12.6708 11.5922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196066_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196066_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196068_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196068_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:55:43.81 +41:06:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196070_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196070_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196081_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196081_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196084_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196084_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196089_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196089_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:26:51.38 +41:14:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.852 194185749313653120 081.71432582030 +41.23551593293 12.8818 11.9356 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 196098_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196098_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196104_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196104_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:58.11 +50:54:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196105_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196105_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:44.71 +46:30:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196110_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196110_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:40.29 +48:57:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196115_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196115_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196118_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196118_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196130_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196130_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:12:10.22 +50:14:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196157_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196157_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196158_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196158_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:28:43.95 +41:18:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.627 194505771619147776 082.18314538158 +41.30272918703 13.1352 12.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196159_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196159_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:02.45 +49:49:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.373 211485533981987968 087.26034393516 +49.83283336790 13.1234 12.2992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196166_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196166_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:40.75 +41:28:16.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196168_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196168_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196170_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196170_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:40:25.90 +48:47:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196175_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196175_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:53.91 +49:47:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196177_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196177_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 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 196182_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196182_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196186_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196186_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:46:42.69 +50:56:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196191_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196191_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:03:15.33 +49:29:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 1.207 970317499685347200 090.81417500874 +49.49589386941 13.2117 12.4205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196193_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196193_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:16.22 +46:04:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.156 197524141490742528 086.81759006937 +46.07959594163 13.1672 12.3251 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 196196_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196196_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196197_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196197_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196199_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196199_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196210_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196210_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196212_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196212_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196215_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196215_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196217_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196217_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196220_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196220_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:23.30 +42:09:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196224_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196224_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196239_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196239_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196241_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196241_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196246_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196246_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196251_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196251_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:11:01.05 +47:29:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.699 969463630123153664 092.75440343000 +47.48730684752 13.3527 12.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196255_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196255_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196260_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196260_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:26:06.77 +46:10:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196262_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196262_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196267_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196267_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:19.74 +47:53:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.512 212214338394071808 080.33245046079 +47.89648151556 13.1631 12.2515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196268_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196268_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196269_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196269_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196277_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196277_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196278_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196278_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:45.36 +50:03:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.650 214503968278402688 086.93910743182 +50.05174986337 13.2156 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196287_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196287_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:57.16 +43:05:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196289_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196289_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196297_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196297_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196303_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196303_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:27:50.44 +42:19:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196312_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196312_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:16:54.08 +43:54:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196313_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196316_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196316_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:18:48.25 +44:06:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.724 207680158599604608 079.70193351269 +44.11312538601 13.3106 12.6161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196322_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196322_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196324_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196324_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196328_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196328_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:42.62 +47:53:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.258 212586385641158912 080.67776024297 +47.89856027064 13.3715 12.5283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196334_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196334_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:17:34.73 +46:23:46.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196335_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196335_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:28:58.88 +43:48:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196340_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196340_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196349_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196349_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:13:42.12 +45:31:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196351_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196351_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196354_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196354_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:15.05 +40:57:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196360_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196360_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:44.79 +44:40:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.204 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196361_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196361_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:47:21.02 +48:12:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196365_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196365_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196387_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196387_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:40:17.76 +46:01:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.213 209531873619402752 085.07265712801 +46.01873463116 13.5312 12.9343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196397_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196397_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:59.35 +46:40:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196399_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196399_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:31:40.43 +42:51:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196403_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196403_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196404_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196404_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:41.22 +48:21:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196405_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196405_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:40:14.29 +50:00:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196409_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196409_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196410_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196410_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196411_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196411_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196415_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196415_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196418_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196418_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196420_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196420_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:23.73 +50:13:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.262 261808836861057408 080.84799330687 +50.23144343721 13.3252 12.3513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196428_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196428_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:46.48 +46:04:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.867 209541769223400064 084.69366740623 +46.06689801652 13.5146 12.8649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196440_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196440_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:55:48.16 +42:30:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:00:13.86 +47:43:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.967 963734830944569856 090.05878481423 +47.72069134482 13.5637 12.7687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196447_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196447_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:41.62 +50:41:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 4.213 261875155450928384 080.42251070654 +50.69932540948 13.4670 12.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196448_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196448_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:52:03.68 +49:32:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196453_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196453_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:22.13 +42:59:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.543 196196824798668032 084.59213941369 +42.99726890424 13.4453 12.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196455_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196455_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196457_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196457_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:06.23 +45:12:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196461_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196461_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196464_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196464_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:18:58.11 +43:42:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.607 207515987770326784 079.74275755653 +43.70229955072 13.6619 12.7892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196473_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196473_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:51.20 +46:21:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196479_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196480_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:30.27 +41:38:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196491_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196492_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196492_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:21.86 +47:52:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196504_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196504_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:59.83 +48:30:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.761 212633522903692800 081.49938027995 +48.50188019747 13.7178 13.0924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196510_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196510_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:59:59.05 +43:51:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196514_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196514_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:45.44 +45:22:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196516_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196516_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196517_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196517_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196519_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196519_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:46.24 +41:46:29.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196525_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196525_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196526_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196526_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196527_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196527_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:39:32.75 +41:57:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196529_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196529_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:57.50 +43:06:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.250 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196531_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196531_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:17:15.73 +41:56:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.463 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196532_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196532_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196533_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196533_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196538_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196538_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196547_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196547_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196552_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196552_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:27:03.65 +46:04:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196554_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196554_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:36:30.31 +43:50:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.386 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196557_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196557_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196565_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196565_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196568_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196568_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196573_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196573_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:02.60 +46:44:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196584_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196584_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196586_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196586_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196591_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196591_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:49.04 +51:04:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196592_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196592_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196606_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196606_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:50.53 +49:49:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196610_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196610_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:52:47.04 +41:21:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196612_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196612_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:17:45.60 +44:42:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196618_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196618_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:52:59.27 +46:57:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196620_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196620_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196621_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196621_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196624_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196624_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196628_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196628_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196630_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196630_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196633_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196633_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196634_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196634_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:28.36 +42:00:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.263 195912429244634624 084.36928975315 +42.01213215946 13.8357 13.3198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196636_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196636_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:52:21.23 +42:50:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196641_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196641_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196646_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196646_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:03:21.23 +42:41:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196651_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196651_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:48:44.80 +49:34:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.813 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196659_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196659_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:03:43.76 +50:12:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196670_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196670_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:31.52 +42:59:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196675_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196675_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:03.04 +49:04:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196676_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196676_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:05.59 +48:44:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196679_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196679_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:22:17.26 +45:05:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196680_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196680_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:36:18.66 +47:12:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.166 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196683_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196683_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:20:38.03 +43:07:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196694_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196694_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:53:28.94 +46:52:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.703 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196695_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196695_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:51.94 +48:16:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.400 212612670840480000 080.96704413027 +48.26814712789 14.0705 13.5224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196698_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196698_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:54.11 +46:06:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196699_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196699_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196701_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196701_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:24.81 +49:14:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196704_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196716_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196716_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196717_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196717_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:40.79 +41:24:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196726_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196726_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:53.33 +46:05:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.808 197005378160950784 089.47179707530 +46.09439219961 14.0011 13.1854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196733_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196733_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196737_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196737_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:44.67 +42:36:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.672 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196740_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196740_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196745_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196745_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196747_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196747_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196753_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196753_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 196757_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196757_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:42:50.74 +48:07:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.880 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196758_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196758_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196767_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196767_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196769_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196769_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196772_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196772_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196773_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196773_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196780_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196780_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196782_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196782_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196783_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196783_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 196784_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196784_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:43.16 +50:10:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.653 213769219633738112 080.92960190688 +50.17639561905 13.7633 12.8802 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 196785_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196785_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:24.78 +44:48:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.506 208086290707268608 081.10372106703 +44.80994290569 13.9169 13.0649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196788_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196788_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:56:00.76 +49:05:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.522 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196793_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196793_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:55:48.16 +42:30:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196794_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196794_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196796_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196796_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:05:26.97 +42:40:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196798_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196802_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196802_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196804_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196804_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:44.13 +47:47:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.833 212218358483551616 079.93457606840 +47.79294561915 13.8506 12.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196806_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196806_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:30.54 +42:26:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196808_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196808_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196814_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196815_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196815_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:12:19.97 +50:12:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.859 971668047856866432 093.08386494890 +50.21036651607 14.0540 13.3189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196818_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196818_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196823_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196823_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196826_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196826_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:35:41.28 +44:16:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196827_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196827_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196832_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196832_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196833_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196833_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:42:16.21 +43:16:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.967 196045745028719488 085.56775371942 +43.27358583012 14.0728 13.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196841_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196841_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196842_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196842_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196848_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196848_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196855_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196855_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:17:15.29 +42:06:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196860_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196860_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196861_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196861_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:10:13.56 +49:41:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.713 970161854365804544 092.55679867882 +49.68720630293 14.1192 13.2925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196862_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196862_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:38.79 +47:49:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.412 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196865_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196865_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:43.57 +49:37:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196872_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196872_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:40:34.22 +46:53:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196883_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196883_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:29.88 +49:54:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.572 971091731965538688 096.62459838265 +49.90271527912 14.1099 13.5701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196889_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196889_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:18:35.23 +46:39:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196893_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196893_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196894_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196894_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196896_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196896_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196897_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196897_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:50:06.54 +46:08:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196899_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196899_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:00.68 +46:20:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.659 208287501334038656 083.50390290064 +46.33909529807 14.0153 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196912_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196912_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:36:07.26 +47:47:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.927 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196916_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196916_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:56.43 +50:48:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.551 215347568575186688 083.23502356000 +50.80367783911 13.8986 12.9550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196917_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196917_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196920_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196920_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:05.06 +42:33:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196927_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196927_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:36:55.36 +45:00:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196940_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196940_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:09:10.28 +42:04:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196943_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196943_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:25.83 +42:58:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196956_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196956_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196958_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196958_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196959_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196959_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196965_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196965_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196969_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196969_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196970_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196970_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196971_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196971_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196972_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196972_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196973_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196973_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:39:00.26 +47:35:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.257 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196976_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196976_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:45.39 +44:42:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196977_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196977_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196985_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196985_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 196988_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 196988_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 196996_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196996_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:54:37.68 +42:21:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196997_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196997_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:25.43 +42:20:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.100 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196999_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 196999_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197006_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197006_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197008_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197008_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:48.66 +48:50:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197015_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197015_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:35:36.53 +50:11:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.204 215075473806779008 083.90235443786 +50.19653993164 14.3478 13.7275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197018_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197018_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197034_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197034_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:36.04 +44:09:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197040_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197040_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197049_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197049_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:28.20 +41:29:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.607 195098034727213568 079.86764726201 +41.49140036355 14.0588 13.0596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197053_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197053_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197063_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197063_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:27:22.60 +49:17:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197067_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197067_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197069_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197069_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197102_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197102_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197104_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197104_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197107_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197107_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197109_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197109_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:53:36.93 +50:13:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197111_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197111_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197120_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197120_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197126_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197126_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197128_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197128_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:20:36.25 +50:54:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197129_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197129_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197131_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197131_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197132_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197132_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:00:25.55 +50:29:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.562 970478273196530176 090.10666370339 +50.49988653180 14.3867 13.8521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197136_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197136_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197144_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197144_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197148_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197148_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197149_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197149_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:47.73 +44:25:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.606 195866387195525760 083.19910170110 +44.42056531235 14.1589 13.3384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197153_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197153_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197161_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197161_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197171_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197171_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197178_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197178_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:19:35.22 +50:11:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197189_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197189_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 197192_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197192_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:29:06.72 +50:13:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197199_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197199_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:42:47.47 +45:58:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197206_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197206_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197213_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197213_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197214_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197214_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197220_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197220_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:12.60 +49:49:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197232_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197232_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:02.74 +50:08:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197235_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197235_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197238_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197238_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197251_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197251_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:39:28.54 +44:57:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.584 964672336406009984 099.86714350284 +44.96142197057 14.5311 13.6655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197253_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197260_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197260_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:53:58.41 +42:30:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197268_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197268_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:54:21.51 +42:55:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.601 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197270_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197270_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197291_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197291_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197295_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197295_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197298_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197298_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197302_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197302_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:46:01.42 +49:53:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.632 991219254384148992 101.50644388813 +49.89019966890 14.4079 13.6620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197304_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197304_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:41:07.39 +47:58:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197317_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197317_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197318_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197318_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:10.10 +48:40:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.494 213067421977566720 079.79145509257 +48.68102005136 14.4921 13.5416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197328_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197328_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197329_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197329_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197335_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197335_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:46.16 +49:43:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.022 970717073378527488 096.44268224399 +49.72986681373 14.6980 14.1083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197340_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197340_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:37:36.81 +40:39:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.896 957273963180268288 099.40406226309 +40.65853586996 14.4000 13.8699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197344_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197344_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197345_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197345_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197346_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197346_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197350_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197350_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:51:07.88 +44:47:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197357_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197357_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197359_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197359_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197362_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197362_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197364_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197364_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197369_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197369_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:36.65 +42:49:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.027 195487605440560384 083.15300665615 +42.83062756194 14.5432 13.9657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197372_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197372_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197385_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197385_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:52.01 +51:08:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 0.643 215361278110871296 083.71690410243 +51.13657417348 14.3956 13.5541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197387_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197387_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:28:29.09 +40:15:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.428 957390511413024512 097.12081470880 +40.26632412079 14.3192 13.6445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197393_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197393_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197413_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197413_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197423_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197423_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197431_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197431_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 197433_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197433_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197434_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197434_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:58:29.54 +42:32:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.094 192430997473995648 089.62341327113 +42.54656773858 14.4466 13.6368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197439_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197439_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:34:12.70 +50:46:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.938 215335714465413632 083.55280392855 +50.77258260477 14.6365 14.0100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197443_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197443_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:02.50 +41:48:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.854 194979356190588416 081.01031162770 +41.81169272764 14.1748 13.0122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197449_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197449_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:13.03 +50:13:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.850 971125473228480896 096.55402464209 +50.21828138308 14.3857 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197454_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197454_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197459_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197459_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:35:08.73 +50:08:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.014 215073446582252160 083.78636334685 +50.14188492665 14.4336 13.5408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197463_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197463_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197464_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197464_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:54.35 +50:17:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.204 261848144399968512 079.97690685320 +50.29554219310 14.5876 13.9065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197470_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197470_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197473_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197473_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:00:27.45 +42:54:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.599 960919050386214528 090.11419266104 +42.91073825498 14.5959 13.7863 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 197480_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197480_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197488_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197489_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197489_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:01.98 +48:44:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.101 213255605968257024 079.75868002516 +48.73860797818 14.4726 13.6938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197498_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197498_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197499_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197499_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:27:56.87 +50:10:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.080 968125764989786880 096.98742676767 +50.17889590464 14.8984 14.5596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197502_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197502_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197505_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197505_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197506_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197506_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197513_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197513_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197516_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197516_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197518_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197518_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197526_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197526_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:47.92 +49:52:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197535_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197535_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:43:50.58 +50:03:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.384 214186930972278016 085.96177695140 +50.05316151460 14.6092 14.0276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197543_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197543_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197549_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197549_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:42:55.47 +47:43:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.894 966886924622535168 100.73086014006 +47.72572712044 14.7540 14.2045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197555_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197555_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:38:24.15 +50:45:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.855 215161888548525312 084.60064233850 +50.76056830171 14.8063 14.2089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197559_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197559_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197561_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197561_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197574_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197574_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197575_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197575_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197579_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197579_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197580_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197580_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197581_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197581_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197589_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197589_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197591_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197591_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197592_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197592_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197595_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197595_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:41:13.08 +49:02:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.325 214063923109515648 085.30501273422 +49.03562759739 14.5425 13.7245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197597_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197597_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197614_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197614_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197615_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197615_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:17.63 +46:15:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197618_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197618_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:04:02.05 +42:01:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197619_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197619_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197622_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197622_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:22.31 +44:07:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.243 959204602520168832 096.34257438144 +44.11709696304 12.9853 11.6271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197628_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197628_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:24:26.85 +42:48:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.655 195269386741701632 081.11206568518 +42.80053313966 14.4658 13.5916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197634_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197634_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:47:42.66 +49:56:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.733 991036185697897728 101.92835542094 +49.94024514629 14.7017 14.1827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197635_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197635_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:47.41 +48:49:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.013 212708534510091264 082.69774851724 +48.83064251930 14.7259 14.1866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197638_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197638_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197648_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197648_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197652_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197652_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197655_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197655_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:42:54.13 +49:15:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.757 967077067118317184 100.72505099314 +49.25074296927 14.8905 14.4174 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 197661_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197661_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197682_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197682_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:19:20.78 +48:06:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.320 212991246438207488 079.83712976723 +48.11351916112 14.6065 13.8981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197687_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197687_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:25:25.76 +49:33:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.314 970708517803708672 096.35776094841 +49.55031825811 14.7467 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197697_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197697_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:47:48.21 +45:07:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.590 197224829514684544 086.95075015175 +45.11662289086 14.6563 13.7935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197702_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197702_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197703_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197703_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197710_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197710_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197723_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197723_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197729_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197729_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197731_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197731_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197738_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197738_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197741_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197745_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197745_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197754_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197754_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197769_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197769_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197771_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197771_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197774_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197774_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:33:45.78 +51:08:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.936 215405945770568320 083.44093436270 +51.13668396575 14.7575 14.1538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197776_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197776_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197777_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197777_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197783_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197783_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197784_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197784_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:17:37.78 +45:53:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.493 211810813331103744 079.40782149310 +45.88888750234 14.4787 13.5581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197788_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197788_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:49:03.45 +50:04:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.169 214494828586459392 087.26467997646 +50.07115740572 14.7759 14.0980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197792_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197792_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197801_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197801_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197806_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197806_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197818_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197818_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:27:21.88 +49:01:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.096 213500182882634624 081.84147124187 +49.02053629752 14.6832 13.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197825_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197825_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197828_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197828_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197835_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197835_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197839_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197839_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197849_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197849_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:07:35.78 +44:11:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.590 962729293201935104 091.89928348734 +44.19880144655 14.6478 14.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197850_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197850_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197858_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197858_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:28.34 +44:23:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.420 195867688568530816 083.11863446201 +44.39103560348 14.6777 14.1772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197867_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197867_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197875_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197875_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:32:47.14 +47:37:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 2.150 209389383783833856 083.19673496233 +47.63110924471 14.8017 14.1777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197878_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197878_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197885_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197885_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:31:40.78 +47:06:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.564 209293863711420544 082.92036266659 +47.11043912409 14.5609 13.6258 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 197889_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197889_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:45:04.10 +44:26:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.912 196429543305907328 086.26763639861 +44.44125573998 14.7902 14.0231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197896_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197896_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197899_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197899_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197900_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197900_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 197921_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197921_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197934_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197934_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197950_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197950_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:03:30.59 +46:27:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.191 963522315963058944 090.87753282894 +46.45115210222 14.7556 14.4748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197976_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 197976_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 197987_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 197987_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:59.18 +46:05:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.068 209155703203888640 080.99675522363 +46.09812834135 14.1555 13.1152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198006_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 198006_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 198009_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198009_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 198011_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198011_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:42:28.14 +47:12:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.825 209914125708261632 085.61786771836 +47.21103146767 14.9387 14.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198013_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198013_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:30:23.24 +48:34:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.794 212667337184084096 082.59703293843 +48.58151769869 14.6221 13.9652 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198017_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198017_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:33:45.57 +51:07:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.673 215405872754834944 083.44059566386 +51.13017118265 14.9393 14.1098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198030_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 198030_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 198033_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198033_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:25:38.33 +43:12:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.563 195701151213613952 081.40978979396 +43.21124418521 14.6043 14.0123 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 198046_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198046_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:29:21.27 +46:16:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.986 209066745840688896 082.33881027676 +46.27385216249 14.5171 13.6686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198056_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198056_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:44:28.40 +42:31:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.161 193031674419463808 086.11877011634 +42.51971519176 14.4802 13.6125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198073_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198073_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:23:41.62 +43:19:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.777 207349102520894592 080.92367698773 +43.33142401779 14.4491 13.8365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198084_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198084_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:55:33.16 +41:34:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.325 192181614493031936 088.88797516362 +41.57018889955 14.8061 14.2795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198088_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 198088_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 198142_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 198142_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:29:42.84 +46:33:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.396 209085231379835904 082.42899258963 +46.55253351000 14.7077 14.1466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 63136_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 63136_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:14:59.11 +46:47:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
Preparing report for the candidate 68332_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
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Considering the candidate 96892_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 96892_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:41:12.81 +44:09:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102378_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 102378_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:37:56.99 +44:41:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41230_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 41230_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:57:23.91 +48:22:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 194441_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 160373_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 160373_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 165639_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 165639_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 15085_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 15085_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 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_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 116770_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:21:29.82 +43:44:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37677_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 37677_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52500_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 52500_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 05:59:44.14 +47:37:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52714_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 52714_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80267_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 80267_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 05201_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308
The candidate 05201_fd_Aur-02-Q1b1x1_2026-04-18_22-49-00_20.00sec_-4.90C_LIGHTs_0308 did not pass the final checks
**** FOUND 06:26:01.75 +50:29:26.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 10s
make_report_in_HTML.sh TOTAL: 345s
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 ####
05:27:04.81 +50:07:24.0
05:45:52.61 +46:58:51.6
05:36:41.33 +45:53:25.6
06:21:18.65 +46:15:22.1
05:44:06.54 +47:04:03.4
05:29:36.83 +46:42:47.4
05:50:10.28 +44:48:36.3
05:51:27.84 +45:11:29.0
05:36:46.54 +42:34:24.3
05:57:10.23 +47:26:38.3
06:40:55.24 +47:18:43.8
06:11:49.31 +44:39:03.4
05:56:13.65 +45:31:10.0
06:12:04.53 +50:30:19.2
05:37:29.61 +43:17:38.4
06:03:36.04 +46:24:19.6
05:39:37.22 +43:14:21.9
05:46:17.02 +43:28:19.3
06:31:45.71 +48:30:01.7
05:38:31.10 +48:42:02.3
05:40:29.51 +46:12:12.4
05:47:56.97 +44:02:17.9
05:57:08.94 +45:23:03.9
06:02:14.20 +47:47:01.6
05:53:31.58 +49:45:35.9
05:32:45.74 +42:29:58.3
05:38:27.37 +41:13:50.8
05:42:20.08 +41:20:38.1
05:27:16.23 +45:33:35.1
06:16:36.29 +44:32:56.2
05:51:38.16 +48:20:10.1
05:50:24.82 +41:49:10.7
06:19:48.11 +46:08:40.5
05:37:23.00 +46:49:18.7
05:56:09.57 +44:18:00.5
05:25:37.72 +45:40:57.3
05:40:02.78 +50:02:05.6
05:18:23.03 +45:25:56.9
05:48:04.12 +43:19:50.6
06:01:58.39 +45:20:37.4
06:26:19.88 +41:59:11.5
06:01:32.42 +47:32:26.5
06:47:21.28 +48:12:02.3
06:07:29.95 +46:55:57.2
05:56:51.38 +48:55:54.0
05:30:09.39 +46:12:57.1
06:08:02.32 +46:40:58.7
05:36:14.53 +43:32:31.6
05:31:00.42 +42:54:53.6
05:34:44.46 +47:20:38.1
05:48:23.25 +49:46:58.9
06:02:32.09 +48:11:24.5
05:35:35.22 +44:15:15.2
05:39:41.70 +50:57:35.9
05:27:26.11 +44:48:52.1
05:49:04.33 +41:17:33.3
06:12:44.97 +47:30:43.5
05:32:56.28 +48:45:36.5
05:25:56.82 +45:50:59.2
05:27:53.85 +46:32:59.5
06:13:29.84 +41:58:07.2
05:19:05.27 +47:54:38.6
05:37:19.50 +44:51:38.3
05:18:53.74 +41:48:41.3
06:24:57.39 +49:09:18.4
05:34:19.16 +44:27:44.6
06:23:09.80 +49:10:00.0
05:30:42.61 +45:28:57.8
06:02:24.69 +48:19:51.7
05:37:52.50 +43:02:35.6
06:46:04.02 +47:20:34.9
05:34:15.77 +44:17:06.1
05:31:09.02 +50:39:11.8
06:10:43.29 +49:06:27.4
05:49:06.64 +47:18:00.6
05:48:55.34 +45:35:44.8
06:10:45.12 +48:16:56.7
05:57:11.94 +42:33:34.2
05:36:40.98 +50:02:54.5
05:39:11.02 +42:46:20.7
05:37:41.30 +45:58:10.0
06:47:02.48 +49:45:30.8
05:58:09.62 +48:37:12.8
05:23:13.49 +46:47:06.4
06:07:54.40 +45:58:50.1
06:10:00.22 +45:32:43.5
05:50:43.29 +44:00:02.2
05:53:04.30 +46:18:47.4
06:09:37.20 +50:22:55.8
06:12:42.95 +45:04:28.7
05:37:47.52 +43:01:00.3
05:39:45.05 +44:19:14.3
05:44:09.94 +51:12:01.5
05:55:10.62 +48:15:53.1
05:53:04.25 +42:45:02.8
05:58:27.49 +43:46:24.6
05:21:58.74 +44:53:04.4
05:29:01.96 +46:51:52.7
05:40:04.67 +46:36:59.5
06:03:36.27 +46:47:53.8
05:29:41.88 +51:06:57.0
06:37:46.13 +49:41:01.9
05:41:40.19 +46:46:08.7
06:47:22.16 +48:09:56.7
05:35:09.15 +46:30:58.0
05:15:58.21 +47:01:15.5
05:53:03.55 +46:38:37.4
05:46:26.20 +40:58:02.5
05:48:36.38 +47:23:35.8
06:18:51.47 +42:37:49.3
06:39:00.30 +48:47:34.0
05:25:35.90 +41:29:39.9
06:27:33.47 +49:14:31.9
06:01:27.32 +41:10:21.2
06:10:25.71 +47:23:33.3
05:44:51.27 +50:14:35.1
06:17:04.73 +47:27:27.7
05:30:57.98 +47:37:05.2
05:26:12.33 +45:06:49.6
05:58:09.08 +49:53:58.1
06:20:20.72 +45:44:44.3
05:30:42.95 +49:02:24.0
05:36:55.83 +47:20:53.1
06:14:29.22 +49:21:03.5
06:36:46.01 +50:00:21.8
06:30:33.50 +48:15:41.4
05:50:49.14 +40:56:46.9
06:13:08.06 +49:47:33.1
05:41:49.04 +50:37:29.7
05:24:32.40 +48:16:54.0
05:23:20.64 +46:37:01.0
06:02:51.55 +46:26:04.8
06:08:46.93 +47:34:13.2
05:56:24.37 +42:43:40.4
05:48:23.06 +47:51:43.9
05:44:45.84 +46:15:16.1
05:35:03.59 +44:14:33.3
05:34:49.19 +44:42:16.3
06:17:58.06 +47:16:18.9
05:50:24.23 +41:50:41.0
05:49:58.99 +42:16:51.0
06:01:08.02 +48:35:19.0
05:30:13.66 +43:45:48.9
06:14:09.54 +45:48:19.1
06:04:20.56 +48:09:19.6
05:49:08.85 +49:16:03.0
05:48:26.39 +41:34:09.1
05:45:26.58 +48:55:44.1
05:40:14.58 +49:56:13.3
05:41:14.23 +46:52:11.2
06:09:51.83 +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 ####
05:27:04.81 +50:07:24.0
05:45:52.61 +46:58:51.6
05:36:41.33 +45:53:25.6
06:21:18.65 +46:15:22.1
05:44:06.54 +47:04:03.4
05:29:36.83 +46:42:47.4
05:50:10.28 +44:48:36.3
05:51:27.84 +45:11:29.0
05:36:46.54 +42:34:24.3
05:57:10.23 +47:26:38.3
06:40:55.24 +47:18:43.8
06:11:49.31 +44:39:03.4
05:56:13.65 +45:31:10.0
06:12:04.53 +50:30:19.2
05:37:29.61 +43:17:38.4
06:03:36.04 +46:24:19.6
05:39:37.22 +43:14:21.9
05:46:17.02 +43:28:19.3
06:31:45.71 +48:30:01.7
05:38:31.10 +48:42:02.3
05:40:29.51 +46:12:12.4
05:47:56.97 +44:02:17.9
05:57:08.94 +45:23:03.9
06:02:14.20 +47:47:01.6
05:53:31.58 +49:45:35.9
05:32:45.74 +42:29:58.3
05:38:27.37 +41:13:50.8
05:42:20.08 +41:20:38.1
05:27:16.23 +45:33:35.1
06:16:36.29 +44:32:56.2
05:51:38.16 +48:20:10.1
05:50:24.82 +41:49:10.7
06:19:48.11 +46:08:40.5
05:37:23.00 +46:49:18.7
05:56:09.57 +44:18:00.5
05:25:37.72 +45:40:57.3
05:40:02.78 +50:02:05.6
05:18:23.03 +45:25:56.9
05:48:04.12 +43:19:50.6
06:01:58.39 +45:20:37.4
06:26:19.88 +41:59:11.5
06:01:32.42 +47:32:26.5
06:47:21.28 +48:12:02.3
06:07:29.95 +46:55:57.2
05:56:51.38 +48:55:54.0
05:30:09.39 +46:12:57.1
06:08:02.32 +46:40:58.7
05:36:14.53 +43:32:31.6
05:31:00.42 +42:54:53.6
05:34:44.46 +47:20:38.1
05:48:23.25 +49:46:58.9
06:02:32.09 +48:11:24.5
05:35:35.22 +44:15:15.2
05:39:41.70 +50:57:35.9
05:27:26.11 +44:48:52.1
05:49:04.33 +41:17:33.3
06:12:44.97 +47:30:43.5
05:32:56.28 +48:45:36.5
05:25:56.82 +45:50:59.2
05:27:53.85 +46:32:59.5
06:13:29.84 +41:58:07.2
05:19:05.27 +47:54:38.6
05:37:19.50 +44:51:38.3
05:18:53.74 +41:48:41.3
06:24:57.39 +49:09:18.4
05:34:19.16 +44:27:44.6
06:23:09.80 +49:10:00.0
05:30:42.61 +45:28:57.8
06:02:24.69 +48:19:51.7
05:37:52.50 +43:02:35.6
06:46:04.02 +47:20:34.9
05:34:15.77 +44:17:06.1
05:31:09.02 +50:39:11.8
06:10:43.29 +49:06:27.4
05:49:06.64 +47:18:00.6
05:48:55.34 +45:35:44.8
06:10:45.12 +48:16:56.7
05:57:11.94 +42:33:34.2
05:36:40.98 +50:02:54.5
05:39:11.02 +42:46:20.7
05:37:41.30 +45:58:10.0
06:47:02.48 +49:45:30.8
05:58:09.62 +48:37:12.8
05:23:13.49 +46:47:06.4
06:07:54.40 +45:58:50.1
06:10:00.22 +45:32:43.5
05:50:43.29 +44:00:02.2
05:53:04.30 +46:18:47.4
06:09:37.20 +50:22:55.8
06:12:42.95 +45:04:28.7
05:37:47.52 +43:01:00.3
05:39:45.05 +44:19:14.3
05:44:09.94 +51:12:01.5
05:55:10.62 +48:15:53.1
05:53:04.25 +42:45:02.8
05:58:27.49 +43:46:24.6
05:21:58.74 +44:53:04.4
05:29:01.96 +46:51:52.7
05:40:04.67 +46:36:59.5
06:03:36.27 +46:47:53.8
05:29:41.88 +51:06:57.0
06:37:46.13 +49:41:01.9
05:41:40.19 +46:46:08.7
06:47:22.16 +48:09:56.7
05:35:09.15 +46:30:58.0
05:15:58.21 +47:01:15.5
05:53:03.55 +46:38:37.4
05:46:26.20 +40:58:02.5
05:48:36.38 +47:23:35.8
06:18:51.47 +42:37:49.3
06:39:00.30 +48:47:34.0
05:25:35.90 +41:29:39.9
06:27:33.47 +49:14:31.9
06:01:27.32 +41:10:21.2
06:10:25.71 +47:23:33.3
05:44:51.27 +50:14:35.1
06:17:04.73 +47:27:27.7
05:30:57.98 +47:37:05.2
05:26:12.33 +45:06:49.6
05:58:09.08 +49:53:58.1
06:20:20.72 +45:44:44.3
05:30:42.95 +49:02:24.0
05:36:55.83 +47:20:53.1
06:14:29.22 +49:21:03.5
06:36:46.01 +50:00:21.8
06:30:33.50 +48:15:41.4
05:50:49.14 +40:56:46.9
06:13:08.06 +49:47:33.1
05:41:49.04 +50:37:29.7
05:24:32.40 +48:16:54.0
05:23:20.64 +46:37:01.0
06:02:51.55 +46:26:04.8
06:08:46.93 +47:34:13.2
05:56:24.37 +42:43:40.4
05:48:23.06 +47:51:43.9
05:44:45.84 +46:15:16.1
05:35:03.59 +44:14:33.3
05:34:49.19 +44:42:16.3
06:17:58.06 +47:16:18.9
05:50:24.23 +41:50:41.0
05:49:58.99 +42:16:51.0
06:01:08.02 +48:35:19.0
05:30:13.66 +43:45:48.9
06:14:09.54 +45:48:19.1
06:04:20.56 +48:09:19.6
05:49:08.85 +49:16:03.0
05:48:26.39 +41:34:09.1
05:45:26.58 +48:55:44.1
05:40:14.58 +49:56:13.3
05:41:14.23 +46:52:11.2
06:09:51.83 +46:34:27.5
###################################################################################
05:27:04.81 +50:07:24.0 -- not an asteroid (will add it to exclusion list)
05:45:52.61 +46:58:51.6 -- not an asteroid (will add it to exclusion list)
05:36:41.33 +45:53:25.6 -- not an asteroid (will add it to exclusion list)
06:21:18.65 +46:15:22.1 -- not an asteroid (will add it to exclusion list)
05:44:06.54 +47:04:03.4 -- not an asteroid (will add it to exclusion list)
05:29:36.83 +46:42:47.4 -- not an asteroid (will add it to exclusion list)
05:50:10.28 +44:48:36.3 -- not an asteroid (will add it to exclusion list)
05:51:27.84 +45:11:29.0 -- not an asteroid (will add it to exclusion list)
05:36:46.54 +42:34:24.3 -- not an asteroid (will add it to exclusion list)
05:57:10.23 +47:26:38.3 -- not an asteroid (will add it to exclusion list)
06:40:55.24 +47:18:43.8 -- not an asteroid (will add it to exclusion list)
06:11:49.31 +44:39:03.4 -- not an asteroid (will add it to exclusion list)
05:56:13.65 +45:31:10.0 -- not an asteroid (will add it to exclusion list)
06:12:04.53 +50:30:19.2 -- not an asteroid (will add it to exclusion list)
05:37:29.61 +43:17:38.4 -- not an asteroid (will add it to exclusion list)
06:03:36.04 +46:24:19.6 -- not an asteroid (will add it to exclusion list)
05:39:37.22 +43:14:21.9 -- not an asteroid (will add it to exclusion list)
05:46:17.02 +43:28:19.3 -- not an asteroid (will add it to exclusion list)
06:31:45.71 +48:30:01.7 -- not an asteroid (will add it to exclusion list)
05:38:31.10 +48:42:02.3 -- not an asteroid (will add it to exclusion list)
05:40:29.51 +46:12:12.4 -- not an asteroid (will add it to exclusion list)
05:47:56.97 +44:02:17.9 -- not an asteroid (will add it to exclusion list)
05:57:08.94 +45:23:03.9 -- not an asteroid (will add it to exclusion list)
06:02:14.20 +47:47:01.6 -- not an asteroid (will add it to exclusion list)
05:53:31.58 +49:45:35.9 -- not an asteroid (will add it to exclusion list)
05:32:45.74 +42:29:58.3 -- not an asteroid (will add it to exclusion list)
05:38:27.37 +41:13:50.8 -- not an asteroid (will add it to exclusion list)
05:42:20.08 +41:20:38.1 -- not an asteroid (will add it to exclusion list)
05:27:16.23 +45:33:35.1 -- not an asteroid (will add it to exclusion list)
06:16:36.29 +44:32:56.2 -- not an asteroid (will add it to exclusion list)
05:51:38.16 +48:20:10.1 -- not an asteroid (will add it to exclusion list)
05:50:24.82 +41:49:10.7 -- not an asteroid (will add it to exclusion list)
06:19:48.11 +46:08:40.5 -- not an asteroid (will add it to exclusion list)
05:37:23.00 +46:49:18.7 -- not an asteroid (will add it to exclusion list)
05:56:09.57 +44:18:00.5 -- not an asteroid (will add it to exclusion list)
05:25:37.72 +45:40:57.3 -- not an asteroid (will add it to exclusion list)
05:40:02.78 +50:02:05.6 -- not an asteroid (will add it to exclusion list)
05:18:23.03 +45:25:56.9 -- not an asteroid (will add it to exclusion list)
05:48:04.12 +43:19:50.6 -- not an asteroid (will add it to exclusion list)
06:01:58.39 +45:20:37.4 -- not an asteroid (will add it to exclusion list)
06:26:19.88 +41:59:11.5 -- not an asteroid (will add it to exclusion list)
06:01:32.42 +47:32:26.5 -- not an asteroid (will add it to exclusion list)
06:47:21.28 +48:12:02.3 -- not an asteroid (will add it to exclusion list)
06:07:29.95 +46:55:57.2 -- not an asteroid (will add it to exclusion list)
05:56:51.38 +48:55:54.0 -- not an asteroid (will add it to exclusion list)
05:30:09.39 +46:12:57.1 -- not an asteroid (will add it to exclusion list)
06:08:02.32 +46:40:58.7 -- not an asteroid (will add it to exclusion list)
05:36:14.53 +43:32:31.6 -- not an asteroid (will add it to exclusion list)
05:31:00.42 +42:54:53.6 -- not an asteroid (will add it to exclusion list)
05:34:44.46 +47:20:38.1 -- not an asteroid (will add it to exclusion list)
05:48:23.25 +49:46:58.9 -- not an asteroid (will add it to exclusion list)
06:02:32.09 +48:11:24.5 -- not an asteroid (will add it to exclusion list)
05:35:35.22 +44:15:15.2 -- not an asteroid (will add it to exclusion list)
05:39:41.70 +50:57:35.9 -- not an asteroid (will add it to exclusion list)
05:27:26.11 +44:48:52.1 -- not an asteroid (will add it to exclusion list)
05:49:04.33 +41:17:33.3 -- not an asteroid (will add it to exclusion list)
06:12:44.97 +47:30:43.5 -- not an asteroid (will add it to exclusion list)
05:32:56.28 +48:45:36.5 -- not an asteroid (will add it to exclusion list)
05:25:56.82 +45:50:59.2 -- not an asteroid (will add it to exclusion list)
05:27:53.85 +46:32:59.5 -- not an asteroid (will add it to exclusion list)
06:13:29.84 +41:58:07.2 -- not an asteroid (will add it to exclusion list)
05:19:05.27 +47:54:38.6 -- not an asteroid (will add it to exclusion list)
05:37:19.50 +44:51:38.3 -- not an asteroid (will add it to exclusion list)
05:18:53.74 +41:48:41.3 -- not an asteroid (will add it to exclusion list)
06:24:57.39 +49:09:18.4 -- not an asteroid (will add it to exclusion list)
05:34:19.16 +44:27:44.6 -- not an asteroid (will add it to exclusion list)
06:23:09.80 +49:10:00.0 -- not an asteroid (will add it to exclusion list)
05:30:42.61 +45:28:57.8 -- not an asteroid (will add it to exclusion list)
06:02:24.69 +48:19:51.7 -- not an asteroid (will add it to exclusion list)
05:37:52.50 +43:02:35.6 -- not an asteroid (will add it to exclusion list)
06:46:04.02 +47:20:34.9 -- not an asteroid (will add it to exclusion list)
05:34:15.77 +44:17:06.1 -- not an asteroid (will add it to exclusion list)
05:31:09.02 +50:39:11.8 -- not an asteroid (will add it to exclusion list)
06:10:43.29 +49:06:27.4 -- not an asteroid (will add it to exclusion list)
05:49:06.64 +47:18:00.6 -- not an asteroid (will add it to exclusion list)
05:48:55.34 +45:35:44.8 -- not an asteroid (will add it to exclusion list)
06:10:45.12 +48:16:56.7 -- not an asteroid (will add it to exclusion list)
05:57:11.94 +42:33:34.2 -- not an asteroid (will add it to exclusion list)
05:36:40.98 +50:02:54.5 -- not an asteroid (will add it to exclusion list)
05:39:11.02 +42:46:20.7 -- not an asteroid (will add it to exclusion list)
05:37:41.30 +45:58:10.0 -- not an asteroid (will add it to exclusion list)
06:47:02.48 +49:45:30.8 -- not an asteroid (will add it to exclusion list)
05:58:09.62 +48:37:12.8 -- not an asteroid (will add it to exclusion list)
05:23:13.49 +46:47:06.4 -- not an asteroid (will add it to exclusion list)
06:07:54.40 +45:58:50.1 -- not an asteroid (will add it to exclusion list)
06:10:00.22 +45:32:43.5 -- not an asteroid (will add it to exclusion list)
05:50:43.29 +44:00:02.2 -- not an asteroid (will add it to exclusion list)
05:53:04.30 +46:18:47.4 -- not an asteroid (will add it to exclusion list)
06:09:37.20 +50:22:55.8 -- not an asteroid (will add it to exclusion list)
06:12:42.95 +45:04:28.7 -- not an asteroid (will add it to exclusion list)
05:37:47.52 +43:01:00.3 -- not an asteroid (will add it to exclusion list)
05:39:45.05 +44:19:14.3 -- not an asteroid (will add it to exclusion list)
05:44:09.94 +51:12:01.5 -- not an asteroid (will add it to exclusion list)
05:55:10.62 +48:15:53.1 -- not an asteroid (will add it to exclusion list)
05:53:04.25 +42:45:02.8 -- not an asteroid (will add it to exclusion list)
05:58:27.49 +43:46:24.6 -- not an asteroid (will add it to exclusion list)
05:21:58.74 +44:53:04.4 -- not an asteroid (will add it to exclusion list)
05:29:01.96 +46:51:52.7 -- not an asteroid (will add it to exclusion list)
05:40:04.67 +46:36:59.5 -- not an asteroid (will add it to exclusion list)
06:03:36.27 +46:47:53.8 -- not an asteroid (will add it to exclusion list)
05:29:41.88 +51:06:57.0 -- not an asteroid (will add it to exclusion list)
06:37:46.13 +49:41:01.9 -- not an asteroid (will add it to exclusion list)
05:41:40.19 +46:46:08.7 -- not an asteroid (will add it to exclusion list)
06:47:22.16 +48:09:56.7 -- not an asteroid (will add it to exclusion list)
05:35:09.15 +46:30:58.0 -- not an asteroid (will add it to exclusion list)
05:15:58.21 +47:01:15.5 -- not an asteroid (will add it to exclusion list)
05:53:03.55 +46:38:37.4 -- not an asteroid (will add it to exclusion list)
05:46:26.20 +40:58:02.5 -- not an asteroid (will add it to exclusion list)
05:48:36.38 +47:23:35.8 -- not an asteroid (will add it to exclusion list)
06:18:51.47 +42:37:49.3 -- not an asteroid (will add it to exclusion list)
06:39:00.30 +48:47:34.0 -- not an asteroid (will add it to exclusion list)
05:25:35.90 +41:29:39.9 -- not an asteroid (will add it to exclusion list)
06:27:33.47 +49:14:31.9 -- not an asteroid (will add it to exclusion list)
06:01:27.32 +41:10:21.2 -- not an asteroid (will add it to exclusion list)
06:10:25.71 +47:23:33.3 -- not an asteroid (will add it to exclusion list)
05:44:51.27 +50:14:35.1 -- not an asteroid (will add it to exclusion list)
06:17:04.73 +47:27:27.7 -- not an asteroid (will add it to exclusion list)
05:30:57.98 +47:37:05.2 -- not an asteroid (will add it to exclusion list)
05:26:12.33 +45:06:49.6 -- not an asteroid (will add it to exclusion list)
05:58:09.08 +49:53:58.1 -- not an asteroid (will add it to exclusion list)
06:20:20.72 +45:44:44.3 -- not an asteroid (will add it to exclusion list)
05:30:42.95 +49:02:24.0 -- not an asteroid (will add it to exclusion list)
05:36:55.83 +47:20:53.1 -- not an asteroid (will add it to exclusion list)
06:14:29.22 +49:21:03.5 -- not an asteroid (will add it to exclusion list)
06:36:46.01 +50:00:21.8 -- not an asteroid (will add it to exclusion list)
06:30:33.50 +48:15:41.4 -- not an asteroid (will add it to exclusion list)
05:50:49.14 +40:56:46.9 -- not an asteroid (will add it to exclusion list)
06:13:08.06 +49:47:33.1 -- not an asteroid (will add it to exclusion list)
05:41:49.04 +50:37:29.7 -- not an asteroid (will add it to exclusion list)
05:24:32.40 +48:16:54.0 -- not an asteroid (will add it to exclusion list)
05:23:20.64 +46:37:01.0 -- not an asteroid (will add it to exclusion list)
06:02:51.55 +46:26:04.8 -- not an asteroid (will add it to exclusion list)
06:08:46.93 +47:34:13.2 -- not an asteroid (will add it to exclusion list)
05:56:24.37 +42:43:40.4 -- not an asteroid (will add it to exclusion list)
05:48:23.06 +47:51:43.9 -- not an asteroid (will add it to exclusion list)
05:44:45.84 +46:15:16.1 -- not an asteroid (will add it to exclusion list)
05:35:03.59 +44:14:33.3 -- not an asteroid (will add it to exclusion list)
05:34:49.19 +44:42:16.3 -- not an asteroid (will add it to exclusion list)
06:17:58.06 +47:16:18.9 -- not an asteroid (will add it to exclusion list)
05:50:24.23 +41:50:41.0 -- not an asteroid (will add it to exclusion list)
05:49:58.99 +42:16:51.0 -- not an asteroid (will add it to exclusion list)
06:01:08.02 +48:35:19.0 -- not an asteroid (will add it to exclusion list)
05:30:13.66 +43:45:48.9 -- not an asteroid (will add it to exclusion list)
06:14:09.54 +45:48:19.1 -- not an asteroid (will add it to exclusion list)
06:04:20.56 +48:09:19.6 -- not an asteroid (will add it to exclusion list)
05:49:08.85 +49:16:03.0 -- not an asteroid (will add it to exclusion list)
05:48:26.39 +41:34:09.1 -- not an asteroid (will add it to exclusion list)
05:45:26.58 +48:55:44.1 -- not an asteroid (will add it to exclusion list)
05:40:14.58 +49:56:13.3 -- not an asteroid (will add it to exclusion list)
05:41:14.23 +46:52:11.2 -- not an asteroid (will add it to exclusion list)
06:09:51.83 +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'
05:15:58.21 +47:01:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:23.03 +45:25:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:53.74 +41:48:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:05.27 +47:54:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:58.74 +44:53:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:13.49 +46:47:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:20.64 +46:37:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:32.40 +48:16:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:35.90 +41:29:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:37.72 +45:40:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:56.82 +45:50:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:12.33 +45:06:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:04.81 +50:07:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:16.23 +45:33:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:26.11 +44:48:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:53.85 +46:32:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:01.96 +46:51:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:36.83 +46:42:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:41.88 +51:06:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:09.39 +46:12:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:13.66 +43:45:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:42.61 +45:28:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:42.95 +49:02:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:57.98 +47:37:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:00.42 +42:54:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:09.02 +50:39:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:45.74 +42:29:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:56.28 +48:45:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.77 +44:17:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.16 +44:27:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:44.46 +47:20:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:49.19 +44:42:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:03.59 +44:14:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:09.15 +46:30:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:35.22 +44:15:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:14.53 +43:32:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.98 +50:02:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:41.33 +45:53:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:46.54 +42:34:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:55.83 +47:20:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.50 +44:51:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:23.00 +46:49:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:29.61 +43:17:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.30 +45:58:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:47.52 +43:01:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.50 +43:02:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.37 +41:13:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:31.10 +48:42:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:11.02 +42:46:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:37.22 +43:14:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:41.70 +50:57:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:45.05 +44:19:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.78 +50:02:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:04.67 +46:36:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:14.58 +49:56:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:29.51 +46:12:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:14.23 +46:52:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:40.19 +46:46:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:49.04 +50:37:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:20.08 +41:20:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:06.54 +47:04:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:09.94 +51:12:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:45.84 +46:15:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:51.27 +50:14:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:26.58 +48:55:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:52.61 +46:58:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:17.02 +43:28:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:26.20 +40:58:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:56.97 +44:02:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:04.12 +43:19:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.06 +47:51:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.25 +49:46:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:26.39 +41:34:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:36.38 +47:23:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:55.34 +45:35:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:04.33 +41:17:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.64 +47:18:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:08.85 +49:16:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:58.99 +42:16:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.28 +44:48:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:24.23 +41:50:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:24.82 +41:49:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:43.29 +44:00:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:49.14 +40:56:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:27.84 +45:11:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:38.16 +48:20:10.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:03.55 +46:38:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.25 +42:45:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.30 +46:18:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:31.58 +49:45:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.62 +48:15:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:09.57 +44:18:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:13.65 +45:31:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:24.37 +42:43:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:51.38 +48:55:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:08.94 +45:23:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:10.23 +47:26:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.94 +42:33:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.08 +49:53:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.62 +48:37:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.49 +43:46:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:08.02 +48:35:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:27.32 +41:10:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:32.42 +47:32:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:58.39 +45:20:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.20 +47:47:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:24.69 +48:19:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.09 +48:11:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:51.55 +46:26:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:36.04 +46:24:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:36.27 +46:47:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:20.56 +48:09:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:29.95 +46:55:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:54.40 +45:58:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:02.32 +46:40:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:46.93 +47:34:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:37.20 +50:22:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:51.83 +46:34:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:00.22 +45:32:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:25.71 +47:23:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:43.29 +49:06:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.12 +48:16:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:49.31 +44:39:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:04.53 +50:30:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:42.95 +45:04:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:44.97 +47:30:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:08.06 +49:47:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.84 +41:58:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:09.54 +45:48:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:29.22 +49:21:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:36.29 +44:32:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:04.73 +47:27:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:58.06 +47:16:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:51.47 +42:37:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:48.11 +46:08:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:20.72 +45:44:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:18.65 +46:15:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:09.80 +49:10:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:57.39 +49:09:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.88 +41:59:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:33.47 +49:14:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:33.50 +48:15:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:45.71 +48:30:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:46.01 +50:00:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:46.13 +49:41:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:00.30 +48:47:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:55.24 +47:18:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:04.02 +47:20:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:02.48 +49:45:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:21.28 +48:12:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:22.16 +48:09:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:15:58.21 +47:01:15.5 -- a known variable star
05:18:23.03 +45:25:56.9 -- not a known variable star
05:18:53.74 +41:48:41.3 -- not a known variable star
05:19:05.27 +47:54:38.6 -- not a known variable star
05:21:58.74 +44:53:04.4 -- a known variable star
05:23:13.49 +46:47:06.4 -- not a known variable star
05:23:20.64 +46:37:01.0 -- not a known variable star
05:24:32.40 +48:16:54.0 -- not a known variable star
05:25:35.90 +41:29:39.9 -- not a known variable star
05:25:37.72 +45:40:57.3 -- not a known variable star
05:25:56.82 +45:50:59.2 -- not a known variable star
05:26:12.33 +45:06:49.6 -- not a known variable star
05:27:04.81 +50:07:24.0 -- a known variable star
05:27:16.23 +45:33:35.1 -- not a known variable star
05:27:26.11 +44:48:52.1 -- not a known variable star
05:27:53.85 +46:32:59.5 -- not a known variable star
05:29:01.96 +46:51:52.7 -- not a known variable star
05:29:36.83 +46:42:47.4 -- not a known variable star
05:29:41.88 +51:06:57.0 -- not a known variable star
05:30:09.39 +46:12:57.1 -- not a known variable star
05:30:13.66 +43:45:48.9 -- not a known variable star
05:30:42.61 +45:28:57.8 -- not a known variable star
05:30:42.95 +49:02:24.0 -- not a known variable star
05:30:57.98 +47:37:05.2 -- not a known variable star
05:31:00.42 +42:54:53.6 -- not a known variable star
05:31:09.02 +50:39:11.8 -- not a known variable star
05:32:45.74 +42:29:58.3 -- not a known variable star
05:32:56.28 +48:45:36.5 -- not a known variable star
05:34:15.77 +44:17:06.1 -- not a known variable star
05:34:19.16 +44:27:44.6 -- not a known variable star
05:34:44.46 +47:20:38.1 -- not a known variable star
05:34:49.19 +44:42:16.3 -- not a known variable star
05:35:03.59 +44:14:33.3 -- not a known variable star
05:35:09.15 +46:30:58.0 -- not a known variable star
05:35:35.22 +44:15:15.2 -- not a known variable star
05:36:14.53 +43:32:31.6 -- not a known variable star
05:36:40.98 +50:02:54.5 -- not a known variable star
05:36:41.33 +45:53:25.6 -- not a known variable star
05:36:46.54 +42:34:24.3 -- not a known variable star
05:36:55.83 +47:20:53.1 -- not a known variable star
05:37:19.50 +44:51:38.3 -- not a known variable star
05:37:23.00 +46:49:18.7 -- not a known variable star
05:37:29.61 +43:17:38.4 -- not a known variable star
05:37:41.30 +45:58:10.0 -- not a known variable star
05:37:47.52 +43:01:00.3 -- not a known variable star
05:37:52.50 +43:02:35.6 -- not a known variable star
05:38:27.37 +41:13:50.8 -- not a known variable star
05:38:31.10 +48:42:02.3 -- not a known variable star
05:39:11.02 +42:46:20.7 -- not a known variable star
05:39:37.22 +43:14:21.9 -- not a known variable star
05:39:41.70 +50:57:35.9 -- not a known variable star
05:39:45.05 +44:19:14.3 -- not a known variable star
05:40:02.78 +50:02:05.6 -- not a known variable star
05:40:04.67 +46:36:59.5 -- not a known variable star
05:40:14.58 +49:56:13.3 -- a known variable star
05:40:29.51 +46:12:12.4 -- not a known variable star
05:41:14.23 +46:52:11.2 -- not a known variable star
05:41:40.19 +46:46:08.7 -- not a known variable star
05:41:49.04 +50:37:29.7 -- not a known variable star
05:42:20.08 +41:20:38.1 -- not a known variable star
05:44:06.54 +47:04:03.4 -- not a known variable star
05:44:09.94 +51:12:01.5 -- not a known variable star
05:44:45.84 +46:15:16.1 -- a known variable star
05:44:51.27 +50:14:35.1 -- not a known variable star
05:45:26.58 +48:55:44.1 -- not a known variable star
05:45:52.61 +46:58:51.6 -- a known variable star
05:46:17.02 +43:28:19.3 -- a known variable star
05:46:26.20 +40:58:02.5 -- not a known variable star
05:47:56.97 +44:02:17.9 -- a known variable star
05:48:04.12 +43:19:50.6 -- not a known variable star
05:48:23.06 +47:51:43.9 -- not a known variable star
05:48:23.25 +49:46:58.9 -- not a known variable star
05:48:26.39 +41:34:09.1 -- not a known variable star
05:48:36.38 +47:23:35.8 -- not a known variable star
05:48:55.34 +45:35:44.8 -- not a known variable star
05:49:04.33 +41:17:33.3 -- not a known variable star
05:49:06.64 +47:18:00.6 -- not a known variable star
05:49:08.85 +49:16:03.0 -- not a known variable star
05:49:58.99 +42:16:51.0 -- not a known variable star
05:50:10.28 +44:48:36.3 -- not a known variable star
05:50:24.23 +41:50:41.0 -- not a known variable star
05:50:24.82 +41:49:10.7 -- not a known variable star
05:50:43.29 +44:00:02.2 -- not a known variable star
05:50:49.14 +40:56:46.9 -- not a known variable star
05:51:27.84 +45:11:29.0 -- a known variable star
05:51:38.16 +48:20:10.1 -- not a known variable star
05:53:03.55 +46:38:37.4 -- not a known variable star
05:53:04.25 +42:45:02.8 -- not a known variable star
05:53:04.30 +46:18:47.4 -- not a known variable star
05:53:31.58 +49:45:35.9 -- not a known variable star
05:55:10.62 +48:15:53.1 -- not a known variable star
05:56:09.57 +44:18:00.5 -- not a known variable star
05:56:13.65 +45:31:10.0 -- not a known variable star
05:56:24.37 +42:43:40.4 -- not a known variable star
05:56:51.38 +48:55:54.0 -- not a known variable star
05:57:08.94 +45:23:03.9 -- not a known variable star
05:57:10.23 +47:26:38.3 -- not a known variable star
05:57:11.94 +42:33:34.2 -- not a known variable star
05:58:09.08 +49:53:58.1 -- not a known variable star
05:58:09.62 +48:37:12.8 -- not a known variable star
05:58:27.49 +43:46:24.6 -- not a known variable star
06:01:08.02 +48:35:19.0 -- not a known variable star
06:01:27.32 +41:10:21.2 -- not a known variable star
06:01:32.42 +47:32:26.5 -- not a known variable star
06:01:58.39 +45:20:37.4 -- not a known variable star
06:02:14.20 +47:47:01.6 -- a known variable star
06:02:24.69 +48:19:51.7 -- not a known variable star
06:02:32.09 +48:11:24.5 -- not a known variable star
06:02:51.55 +46:26:04.8 -- not a known variable star
06:03:36.04 +46:24:19.6 -- not a known variable star
06:03:36.27 +46:47:53.8 -- not a known variable star
06:04:20.56 +48:09:19.6 -- not a known variable star
06:07:29.95 +46:55:57.2 -- not a known variable star
06:07:54.40 +45:58:50.1 -- not a known variable star
06:08:02.32 +46:40:58.7 -- not a known variable star
06:08:46.93 +47:34:13.2 -- not a known variable star
06:09:37.20 +50:22:55.8 -- not a known variable star
06:09:51.83 +46:34:27.5 -- a known variable star
06:10:00.22 +45:32:43.5 -- not a known variable star
06:10:25.71 +47:23:33.3 -- not a known variable star
06:10:43.29 +49:06:27.4 -- not a known variable star
06:10:45.12 +48:16:56.7 -- not a known variable star
06:11:49.31 +44:39:03.4 -- not a known variable star
06:12:04.53 +50:30:19.2 -- not a known variable star
06:12:42.95 +45:04:28.7 -- not a known variable star
06:12:44.97 +47:30:43.5 -- not a known variable star
06:13:08.06 +49:47:33.1 -- not a known variable star
06:13:29.84 +41:58:07.2 -- not a known variable star
06:14:09.54 +45:48:19.1 -- not a known variable star
06:14:29.22 +49:21:03.5 -- not a known variable star
06:16:36.29 +44:32:56.2 -- a known variable star
06:17:04.73 +47:27:27.7 -- not a known variable star
06:17:58.06 +47:16:18.9 -- not a known variable star
06:18:51.47 +42:37:49.3 -- not a known variable star
06:19:48.11 +46:08:40.5 -- not a known variable star
06:20:20.72 +45:44:44.3 -- not a known variable star
06:21:18.65 +46:15:22.1 -- not a known variable star
06:23:09.80 +49:10:00.0 -- not a known variable star
06:24:57.39 +49:09:18.4 -- not a known variable star
06:26:19.88 +41:59:11.5 -- not a known variable star
06:27:33.47 +49:14:31.9 -- not a known variable star
06:30:33.50 +48:15:41.4 -- not a known variable star
06:31:45.71 +48:30:01.7 -- a known variable star
06:36:46.01 +50:00:21.8 -- not a known variable star
06:37:46.13 +49:41:01.9 -- not a known variable star
06:39:00.30 +48:47:34.0 -- not a known variable star
06:40:55.24 +47:18:43.8 -- not a known variable star
06:46:04.02 +47:20:34.9 -- not a known variable star
06:47:02.48 +49:45:30.8 -- not a known variable star
06:47:21.28 +48:12:02.3 -- not a known variable star
06:47:22.16 +48:09:56.7 -- not a known variable star
Found 138 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
151 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 151 (excluding asteroids and hot pixels, 138 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461149.65853236 -observatory V36
00:24:27.19 -00:13:18.8 Mercury (-0.1mag)
03:24:10.96 +19:00:07.5 Venus (-3.9mag)
00:26:48.30 +01:50:57.7 Mars (1.2mag)
07:14:07.11 +22:43:45.4 Jupiter (-2.1mag)
00:30:34.85 +00:57:41.0 Saturn (0.9mag)
03:48:22.24 +19:49:37.7 Uranus (5.8mag)
00:11:14.95 -00:12:48.0 Neptune (7.8mag)
20:33:52.96 -22:52:46.8 Pluto (14.5mag)
03:08:48.54 +22:20:49.7 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 362 Apr 18 22:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461149.65853236:
07:13:59.61 +22:44:00.9 Io (5.8mag)
07:14:01.82 +22:43:59.4 Europa (5.9mag)
07:13:47.81 +22:44:26.7 Ganymede (5.4mag)
07:14:22.81 +22:43:04.2 Callisto (6.6mag)
07:17:18.71 +22:29:57.4 Himalia (15.4mag)
07:14:09.73 +22:43:41.3 Thebe (16.2mag)
07:17:33.97 +23:00:17.0 Elara (17.3mag)
07:13:12.88 +23:22:06.6 Pasiphae (17.4mag)
07:22:22.48 +22:42:04.5 Carme (18.5mag)
00:30:25.94 +00:58:02.8 Titan (8.8mag)
00:30:34.03 +00:57:57.1 Rhea (10.1mag)
00:30:10.12 +00:57:20.0 Iapetus (11.5mag)
00:30:30.92 +00:58:09.0 Hyperion (14.8mag)
00:32:09.19 +01:06:08.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 18 22:53 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461149.65853236:
15:51:41.37 -18:22:34.0 JWST
16:14:04.73 +50:00:03.1 Chandra
17:22:55.27 -47:06:47.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 18 22:53 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461149.65853236 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:10.76 -28:58:06.2 13.9mag P/2010 H2 (Vales)
05:09:02.91 -69:30:55.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:09.44 +31:27:34.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:04.19 +10:55:06.7 17.6mag C/2021 G2 (ATLAS)
23:11:01.54 +29:21:25.8 17.1mag C/2022 E2 (ATLAS)
04:32:56.31 +26:07:21.8 16.0mag C/2022 N2 (PANSTARRS)
09:04:10.11 +32:01:47.3 16.2mag C/2022 QE78 (ATLAS)
08:31:36.73 +00:10:30.8 17.4mag C/2022 R6 (PANSTARRS)
18:52:55.26 +18:47:40.3 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:36.72 -11:28:30.3 17.5mag P/2023 B1 (PANSTARRS)
09:06:15.55 -11:23:06.5 17.7mag C/2023 F3 (ATLAS)
21:57:15.86 +63:05:45.6 17.5mag C/2023 H5 (Lemmon)
19:16:17.56 -03:47:25.7 14.1mag C/2023 R1 (PANSTARRS)
21:24:22.55 +86:21:13.6 17.8mag C/2023 X2 (Lemmon)
06:19:30.86 +63:30:10.8 17.2mag C/2024 A1 (ATLAS)
05:19:55.58 +19:18:24.3 11.3mag C/2024 E1 (Wierzchos)
16:17:11.20 +06:54:21.5 17.4mag C/2024 G6 (ATLAS)
20:21:37.33 +16:08:29.4 14.6mag C/2024 J3 (ATLAS)
03:29:13.78 -21:54:40.3 16.3mag C/2024 T5 (ATLAS)
05:19:25.62 +44:31:14.7 17.7mag C/2025 J1 (Borisov)
13:25:50.13 +47:21:08.0 15.3mag C/2025 L1 (ATLAS)
03:30:20.90 -26:42:54.4 17.9mag C/2025 Q3 (ATLAS)
00:18:06.77 +17:01:00.0 8.1mag C/2025 R3 (PANSTARRS)
12:52:45.81 +03:12:00.8 17.4mag C/2025 Y1 (ATLAS)
03:51:22.54 +02:19:58.9 14.2mag C/2026 A1 (MAPS)
00:08:24.54 +37:46:48.5 14.7mag C/2026 B2 (Sun-Gao)
18:49:04.49 -09:32:51.9 11.6mag 10P/Tempel
14:55:59.97 +02:51:51.4 14.3mag 24P/Schaumasse
11:02:00.57 -01:25:40.7 15.7mag 29P/Schwassmann-Wachmann
10:37:33.59 -03:51:32.8 17.0mag 43P/Wolf-Harrington
01:53:34.25 +18:01:21.7 17.3mag 47P/Ashbrook-Jackson
07:16:40.54 +36:19:40.4 17.0mag 63P/Wild
23:33:02.96 -11:04:32.5 15.7mag 65P/Gunn
04:11:46.71 +22:19:07.2 15.9mag 76P/West-Kohoutek-Ikemura
01:12:35.17 +08:50:45.9 14.3mag 78P/Gehrels
23:12:27.80 -08:27:23.2 14.7mag 88P/Howell
02:19:24.85 +21:28:15.7 15.1mag 93P/Lovas
05:00:50.42 +32:27:00.5 16.2mag 123P/West-Hartley
08:32:12.86 +36:54:21.2 16.2mag 124P/Mrkos
02:38:07.16 +14:43:08.4 16.4mag 128P/Shoemaker-Holt
02:53:44.92 +14:52:18.0 17.5mag 131P/Mueller
01:42:54.32 +14:17:14.8 10.5mag 141P/Machholz
01:51:21.04 +06:03:07.3 10.5mag 141P-A/Machholz
00:35:13.86 +01:51:56.5 12.4mag 141P-D/Machholz
02:21:52.80 +07:48:27.9 17.9mag 141P-I/Machholz
01:11:12.77 +00:04:02.4 15.0mag 162P/SidingSpring
14:45:50.89 +00:14:18.2 17.7mag 210P/Christensen
21:47:46.54 -10:41:29.3 17.7mag 218P/LINEAR
17:17:09.32 -13:32:58.7 16.1mag 235P/LINEAR
05:41:21.05 +34:55:26.6 16.8mag 240P/NEAT
07:40:06.99 -04:50:02.3 17.8mag 242P/Spahr
22:24:48.58 -20:07:17.2 17.8mag 260P/McNaught
02:04:41.42 +21:15:04.0 18.0mag 295P/LINEAR
15:41:21.06 +07:11:32.3 17.5mag 391P/Kowalski
07:35:28.46 +21:22:20.6 17.7mag 450P/LONEOS
05:40:31.51 +44:50:53.7 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 18 22:53 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
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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 18 22:53 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:08:30.580 +41:56:13.61 AT 2026jje 2026-04-03.89 21.47
16:48:25.780 +33:00:44.35 AT 2026jjd 2026-04-03.85 21.29
16:46:02.450 +30:55:42.15 AT 2026jjc 2026-04-03.80 19.57
16:51:04.120 +44:26:50.06 AT 2026jjb 2026-03-30.84 21.02
12:10:02.030 +43:26:37.06 AT 2026jja 2026-03-28.87 21.46
17:56:59.910 +48:20:04.31 AT 2026jiz 2026-03-27.87 20.99
15:23:12.550 +15:30:01.81 AT 2026jiy 2026-03-27.82 21.09
12:45:41.400 +53:52:15.13 AT 2026jix 2026-03-24.70 20.56
12:05:28.040 +47:18:05.03 AT 2026jiw 2026-03-24.69 20.17
12:49:49.680 +44:27:28.62 AT 2026jiv 2026-03-24.69 21.87
12:17:57.600 +45:03:04.77 AT 2026jiu 2026-03-24.69 20.4
11:39:16.940 +45:15:03.67 AT 2026jit 2026-03-24.66 21.06
14:17:33.100 +43:22:03.41 AT 2026jis 2026-03-22.80 20.74
14:45:33.130 +38:26:13.04 AT 2026jir 2026-03-22.80 21.14
14:42:55.800 +38:18:34.13 AT 2026jiq 2026-03-22.80 21.14
12:43:36.900 +28:13:26.06 AT 2026jip 2026-03-20.69 21.81
13:50:42.590 +38:45:33.09 AT 2026jio 2026-03-29.93 20.87
19:45:48.257 -49:40:35.86 AT 2026jin 2026-04-12.35 18.142
23:14:08.648 +35:53:12.54 AT 2026jim 2026-03-28.53 17.909
07:22:52.030 +11:04:39.45 AT 2026jil 2026-04-11.54 18.4
-rw-r--r-- 1 apache apache 30K Apr 18 22:53 tns_transients_list.txt
