This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD
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
Gaia DR3 197035717811398528,2461146.6467,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197035717811398528 20260416.1467 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,2461146.6467,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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
ASASSN-V J055127.94+451129.9,2461146.6467,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055127.94+451129.9 20260416.1467 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.8488+47.5605,2461146.6467,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J092.8488+47.5605 20260416.1467 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J084.6117+43.0453,2461146.6467,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6117+43.0453 20260416.1467 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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
ATO J084.5753+42.6040,2461146.6467,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.5753+42.6040 20260416.1467 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209684259058288384,2461146.6467,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209684259058288384 20260416.1467 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 J086.1652+43.4191,2461146.6467,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.1652+43.4191 20260416.1467 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J090.0739+43.2923,2461146.6467,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.0739+43.2923 20260416.1467 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 J085.4610+42.3911,2461146.6467,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.4610+42.3911 20260416.1467 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 965843075770792448,2461146.6467,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 965843075770792448 20260416.1467 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.3839+50.2299,2461146.6467,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.3839+50.2299 20260416.1467 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208009393611989504,2461146.6467,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 208009393611989504 20260416.1467 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.9297+43.1685,2461146.6467,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.9297+43.1685 20260416.1467 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.1681+42.8723,2461146.6467,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.1681+42.8723 20260416.1467 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461146.6467,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197994904265884544 20260416.1467 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1740+42.4269,2461146.6467,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.1740+42.4269 20260416.1467 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 J093.3290+41.8878,2461146.6467,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3290+41.8878 20260416.1467 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J095.3673+41.8196,2461146.6467,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.3673+41.8196 20260416.1467 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 J087.5437+43.6538,2461146.6467,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.5437+43.6538 20260416.1467 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 961627926147988224,2461146.6467,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 961627926147988224 20260416.1467 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963145561432116096,2461146.6467,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963145561432116096 20260416.1467 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053755.31+425401.9,2461146.6467,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053755.31+425401.9 20260416.1467 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 958381892944100352,2461146.6467,9.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 958381892944100352 20260416.1467 9.68CV 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 196564783236506368,2461146.6467,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196564783236506368 20260416.1467 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196796848908972032,2461146.6467,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196796848908972032 20260416.1467 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196143842081588352,2461146.6467,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196143842081588352 20260416.1467 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VV Aur,2461146.6467,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VV Aur 20260416.1467 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461146.6467,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211485843219678720 20260416.1467 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461146.6467,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3195+44.0466 20260416.1467 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 197388553666998656,2461146.6467,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197388553666998656 20260416.1467 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.8541+42.6555,2461146.6467,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.8541+42.6555 20260416.1467 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
target,2461146.6467,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 196552271996570368,2461146.6467,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196552271996570368 20260416.1467 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461146.6467,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2776+47.3006 20260416.1467 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461146.6467,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.1629+50.0440 20260416.1467 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4626+44.3866,2461146.6467,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.4626+44.3866 20260416.1467 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 197161641956644864,2461146.6467,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197161641956644864 20260416.1467 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6503+44.5028,2461146.6467,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.6503+44.5028 20260416.1467 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
ZTF J060033.67+471756.0,2461146.6467,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J060033.67+471756.0 20260416.1467 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5381+48.6224,2461146.6467,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.5381+48.6224 20260416.1467 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.0089+45.8985,2461146.6467,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.0089+45.8985 20260416.1467 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210540155843380736,2461146.6467,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210540155843380736 20260416.1467 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 193198108695286528,2461146.6467,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193198108695286528 20260416.1467 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210216624548997760,2461146.6467,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210216624548997760 20260416.1467 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196792068609390976,2461146.6467,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196792068609390976 20260416.1467 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 J085.3760+42.2915,2461146.6467,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.3760+42.2915 20260416.1467 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,2461146.6467,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J086.9027+45.2906,2461146.6467,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.9027+45.2906 20260416.1467 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970195561269058176,2461146.6467,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 970195561269058176 20260416.1467 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.1141+45.3000,2461146.6467,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.1141+45.3000 20260416.1467 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,2461146.6467,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1139+42.7270,2461146.6467,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1139+42.7270 20260416.1467 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J083.8142+48.1725,2461146.6467,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.8142+48.1725 20260416.1467 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
Gaia DR3 195947132580142080,2461146.6467,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195947132580142080 20260416.1467 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.3462+41.7479,2461146.6467,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.3462+41.7479 20260416.1467 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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 J084.3607+43.4394,2461146.6467,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3607+43.4394 20260416.1467 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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,2461146.6467,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3299+44.4181,2461146.6467,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3299+44.4181 20260416.1467 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 J086.8262+42.3537,2461146.6467,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.8262+42.3537 20260416.1467 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210084996686630656,2461146.6467,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210084996686630656 20260416.1467 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.2989+44.9120,2461146.6467,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.2989+44.9120 20260416.1467 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963190229091955584,2461146.6467,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963190229091955584 20260416.1467 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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,2461146.6467,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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,2461146.6467,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6467,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1467 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
ATO J086.1375+44.0769,2461146.6467,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.1375+44.0769 20260416.1467 14.12CV 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 J096.8783+42.8003,2461146.6467,10.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.8783+42.8003 20260416.1467 10.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461146.64693005 16.04.2026 03:31:24.756 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
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): 16539
Objects passed selection criteria: 16518
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: 15050.2
Average stars matched: 14649.8 (97.3389 %)
Memory usage VmPeak: 122840 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 22:55:26 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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461146.64693005 16.04.2026 03:31:24.756 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 359
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 182 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): 126415
Objects passed selection criteria: 126035
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: 114944
Average stars matched: 110702 (96.3091 %)
Memory usage VmPeak: 1960412 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:00:12 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461146.64639352
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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:31.621 +45:59:46.35 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 06:00:31.621 +45:59:46.35
Angular distance between the image centers 0.1275 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:31.143 +46:00:14.90 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 06:00:31.143 +46:00:14.90
Angular distance between the image centers 0.1255 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 06:00:31.621 +45:59:46.35
Second-epoch second image center 06:00:31.143 +46:00:14.90
Angular distance between the image centers 0.00805 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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.Eg0HjWkNA2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.rDg2t28gHl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.ZTT4sksoK1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits &> /tmp/tmp.bei9p8ChEJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_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 11 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.6 pix fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
2.6 pix fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
15.0 mag. fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
15.0 mag. fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
All-image limiting magnitude estimate: 15.0 (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.Eg0HjWkNA2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.rDg2t28gHl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.ZTT4sksoK1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1432, passed=18836
Got 18836 stars (including 17386 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 18836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 18558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 18556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 18556 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.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.bei9p8ChEJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1507, passed=18882
Got 18882 stars (including 17355 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 18882 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 18603 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 18600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 18600 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31430.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31046_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31046_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:46.25 +43:34:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31049_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31049_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:27.60 +42:19:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31148_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31148_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:14:59.02 +46:47:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31157_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31157_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:28.51 +43:00:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31189_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31189_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:22.97 +46:49:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31263_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31263_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31358_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31358_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:06:11.31 +47:25:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.409 969681535286381312 091.54712051726 +47.42216425873 12.0045 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31367_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31367_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:55:20.96 +43:16:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.220 193310160099657216 088.83737940998 +43.28199553885 12.1323 11.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31370_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31370_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:06:32.55 +48:42:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.777 969672464315450752 091.63600844831 +48.71267373519 12.0182 11.4092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31383_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31383_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:58:17.10 +48:16:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.536 210181474534722688 089.57137503990 +48.26815441263 12.2509 11.7274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31430_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 31430_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:28:45.88 +48:34:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.217 967547868550025216 097.19110438442 +48.57701626020 12.2587 11.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:31.621 +45:59:46.35 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 06:00:31.621 +45:59:46.35
Angular distance between the image centers 0.1275 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:31.143 +46:00:14.90 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 06:00:31.143 +46:00:14.90
Angular distance between the image centers 0.1255 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 06:00:31.621 +45:59:46.35
Second-epoch second image center 06:00:31.143 +46:00:14.90
Angular distance between the image centers 0.00805 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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.DY72QK5iEA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.z2oVzdPCLw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.RLXFIKqeXb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits &> /tmp/tmp.fsN4AGB6b2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_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.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 270 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.1 pix fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.1 mag. fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
14.1 mag. fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
All-image limiting magnitude estimate: 14.1 (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.DY72QK5iEA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.z2oVzdPCLw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_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=44, blended=20075, passed=170060
Got 170060 stars (including 149712 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170060 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166998 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(), 166995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166995 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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_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-Q2b1x1_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.RLXFIKqeXb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=14047, passed=133813
Got 133813 stars (including 119624 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 133813 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 940 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(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 131574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 940 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(), 131573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 131573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.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.fsN4AGB6b2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=13866, passed=132132
Got 132132 stars (including 118143 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 132132 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 129369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 129369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 129368 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.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-Q2b1x1_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_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_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_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-30-38_20.00sec_-5.00C_LIGHT_0093.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Aur-02-Q2b1x1_225248_TTUQ2b1x1_6931_siAhj9rD/wcs_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out192171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out143438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192479.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195295.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 152s
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: 65s
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Considering the candidate 192171_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192171_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:58:04.16 +45:09:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.788 196718268187273216 089.51756371719 +45.16014659211 14.8726 14.2946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192192_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192192_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:46.45 +42:34:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.751 194686370700914176 084.19336771424 +42.57383043954 14.6898 13.8832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192204_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192204_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:24.42 +42:13:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.919 192971613596899456 086.10141863353 +42.21858237723 14.5341 13.6420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192209_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192209_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192210_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192210_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:22.86 +43:10:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.873 193307720558349440 088.59485147135 +43.16776963318 14.7174 13.9676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192214_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192214_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192221_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192221_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:48:34.87 +49:14:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.287 211401009026016128 087.14532316104 +49.24947863643 14.7578 13.8991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192223_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192223_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192224_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192224_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192227_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192227_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:23.05 +43:49:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.153 197044513904385792 084.84612153999 +43.82931500322 14.4859 13.7138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192234_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192234_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192250_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192250_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:56:51.10 +43:51:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.443 193527004408029696 089.21254198087 +43.85779592213 14.5463 13.8053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192255_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192255_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:33.06 +42:10:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.053 192938525169012864 085.13751302577 +42.18101601159 14.6560 14.0186 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:25.54 +44:20:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.734 197095881712708992 085.35634073846 +44.34044664360 14.6309 13.8836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192264_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192264_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:59:30.24 +43:13:17.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 192265_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192265_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:38.69 +42:06:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.139 195913941073058560 084.66091162053 +42.10339409690 14.5192 13.6948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192267_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192267_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192268_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192268_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192279_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192279_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192294_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192294_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:41.27 +46:18:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.003 209724837909062912 084.17226447220 +46.31401483209 14.4137 13.5100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192298_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192298_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:53:01.54 +45:44:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.722 197641273839020800 088.25666431788 +45.73843479968 14.6222 13.7901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192301_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192301_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192304_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192304_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192312_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192312_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:08.57 +44:17:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.463 196424767302324992 085.78543757688 +44.29824609270 14.2401 13.4191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192324_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192324_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192346_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192346_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192350_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192350_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192351_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192351_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192352_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192352_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192358_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192358_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192361_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192361_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:31.14 +48:42:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.657 213958919749204480 084.62958550835 +48.70047503109 14.3458 13.5410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192366_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192366_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:54.92 +41:54:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192368_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192368_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:47:48.86 +43:07:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192371_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192371_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:29.54 +43:17:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.162 196264994519285248 084.37347692679 +43.29464769469 14.4390 13.5734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192372_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192372_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192380_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192380_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:24.60 +44:48:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192382_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192382_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192383_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192383_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:52:15.79 +45:47:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.549 197651169443704448 088.06544000779 +45.79052007687 14.2561 13.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192384_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192384_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:46:17.14 +43:28:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192385_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192385_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192391_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192391_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 192396_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192396_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:36.60 +42:33:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.930 193172858585074688 087.65278292121 +42.56656933705 13.7861 13.1493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192403_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192403_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:30.81 +42:27:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.562 193027723049634176 085.87779610467 +42.45943775910 14.1405 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192408_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192408_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:33.03 +42:15:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192413_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192413_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:40.58 +44:00:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192414_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192414_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:27.01 +43:07:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192416_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192416_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192418_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192418_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192420_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192420_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:47:50.44 +43:23:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.161 196094638936759168 086.96020415910 +43.39040464429 14.0631 13.4533 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 192425_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192425_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192430_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192430_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192432_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192432_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:48:13.28 +42:46:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.210 193015422263418880 087.05560519982 +42.77852047107 13.8801 13.2001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192442_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192442_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:33.52 +43:55:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.697 196319351625187968 085.13972666783 +43.93102191949 13.7275 12.9554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192445_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192445_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:36.89 +46:43:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192454_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192454_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192456_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192456_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192457_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192457_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192460_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192460_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192466_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192466_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:34:44.56 +47:20:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192474_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192474_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:05:21.59 +49:16:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.563 970258577029613440 091.33984605701 +49.28188821276 13.4317 12.6470 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 192475_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192475_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:25.01 +48:02:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192478_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192478_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:50.43 +44:24:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192479_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192479_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192481_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192481_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:31:06.92 +48:10:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192485_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192485_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:25.54 +48:47:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.811 211054628503561472 085.10634246196 +48.79946990081 13.1644 12.4314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192486_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192486_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:43.12 +46:13:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.371 197888973193024896 087.68013303510 +46.21714659712 13.2634 12.3569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192488_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192488_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:01.73 +46:28:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192489_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192489_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:13.16 +47:02:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192492_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192492_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192496_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192496_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:47.96 +41:45:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192498_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192498_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:57.65 +44:20:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.325 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 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 192499_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192499_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192501_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192501_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:20:13.38 +43:38:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.563 961773886316261504 095.05528574915 +43.64410819835 12.5992 12.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192503_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192503_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:13.77 +44:08:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192504_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192504_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:03.09 +42:12:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192506_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192506_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:23.55 +49:53:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192507_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192507_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:17.47 +42:28:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192509_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192509_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:42.27 +43:39:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.195 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192510_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192510_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:24.92 +41:49:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192511_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192511_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:23.77 +44:31:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192512_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192512_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192515_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192515_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:46.00 +43:34:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192517_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192517_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:09.15 +46:13:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192518_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192518_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:21:02.41 +42:34:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 2.146 961574629896597248 095.25955605192 +42.57822680161 11.6010 11.2694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192520_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 192520_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 192521_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192521_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:27.58 +42:19:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192620_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192620_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:28.52 +43:00:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192652_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192652_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:23.02 +46:49:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192749_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192749_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:40.68 +46:06:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 1.509 197582312527881728 086.17009328825 +46.10921892373 11.5038 10.4275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192755_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192755_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:42.97 +43:37:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192851_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192851_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:19.56 +42:40:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192918_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 192918_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:46:26.52 +47:55:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193035_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193035_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:17.79 +45:03:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193076_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193076_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193101_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193101_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:02.85 +50:02:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193106_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193106_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:07.69 +44:53:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193166_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193166_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:51:18.35 +46:14:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193176_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193176_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:02.52 +49:49:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193210_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193210_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:05:50.19 +44:39:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:48:04.17 +43:19:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193284_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193284_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193310_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193310_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193378_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193378_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:52.92 +47:06:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193405_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193405_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:46.38 +43:03:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193426_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193426_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193463_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193463_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:14.32 +50:00:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193476_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193476_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:47:45.39 +50:03:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193499_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193499_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:17.65 +46:01:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193504_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193504_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:34.77 +46:23:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193507_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193507_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:11:01.07 +47:29:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193515_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193515_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:44.85 +44:40:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.932 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193534_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193534_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:24.43 +42:59:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193557_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193557_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:28.30 +42:14:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193590_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193590_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:46.49 +46:04:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193605_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193605_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:52:03.73 +49:32:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193609_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193609_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193616_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193616_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193632_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193632_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:30.10 +44:44:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193636_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193636_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:32.78 +41:57:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193647_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193647_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:22.12 +42:59:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193656_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193656_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:00:14.06 +47:43:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193680_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193680_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193681_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193681_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:18.66 +44:01:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193687_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193687_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:39.85 +43:57:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193734_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193734_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:35:30.63 +45:58:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193740_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193740_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:16.02 +41:56:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.014 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193762_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193762_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193771_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193771_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:52:21.37 +42:50:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193802_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193802_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193804_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193804_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:27.91 +47:51:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.803 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193805_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193805_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:46:39.82 +43:21:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.600 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193813_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193813_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:14.98 +43:32:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193817_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193817_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:50.91 +48:07:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.149 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193822_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193822_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:40:59.60 +46:21:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193846_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193846_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:51:18.91 +43:17:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.335 193427528667708288 087.82879815788 +43.29576806055 13.9092 13.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193848_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193848_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:44.17 +41:49:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193864_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193864_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:48:44.77 +49:34:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.616 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193867_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193867_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:44.76 +42:36:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.464 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193872_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193872_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:35:41.38 +44:16:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193883_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193883_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:52.91 +44:39:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.974 197198582969731584 085.72056700350 +44.66320375605 13.9867 13.3740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193896_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193896_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:50.49 +49:49:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193933_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193933_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193938_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193938_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:53:58.76 +46:09:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193957_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 193957_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 193959_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193959_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:08:19.32 +41:46:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193993_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193993_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:57.57 +42:25:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193994_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 193994_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:35:30.93 +48:04:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194000_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194000_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:18.83 +47:12:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.603 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194006_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194006_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:53.36 +46:05:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194011_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194011_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:30.32 +43:50:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.451 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194037_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194037_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:16.26 +43:16:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194050_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194050_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:38.76 +47:49:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.088 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194057_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194057_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194062_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194062_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:07.36 +47:47:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.328 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194074_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194074_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194098_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194098_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194104_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194104_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194109_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194109_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:24.86 +49:14:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.098 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194116_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194116_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:36:55.54 +45:00:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194119_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194119_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:24.07 +41:41:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194123_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194123_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:24.81 +43:50:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194129_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194129_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:12:19.82 +50:12:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194138_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194138_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:53:28.98 +46:52:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.154 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194141_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194141_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:06.65 +46:08:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194171_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194171_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194172_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194172_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:25:45.41 +45:22:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194178_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194178_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:15.74 +45:20:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194195_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194195_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:40.19 +42:55:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194197_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194197_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:25.62 +42:20:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.785 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194222_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194222_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194227_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194227_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:23.48 +49:49:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.755 214254619657430144 084.84769115489 +49.82477197399 14.0502 13.3596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194232_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194232_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:59.97 +47:35:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.323 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194237_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194237_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:47:11.04 +46:03:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.309 197523351216767360 086.79557643499 +46.05504755708 14.1430 13.2999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194255_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194255_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:33.95 +49:48:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.171 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194259_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 194297_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194297_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194301_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194301_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:17:15.25 +42:06:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194328_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194328_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194351_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194351_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:41.32 +45:58:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.846 209519229235054976 084.42186246455 +45.96920303700 14.2850 13.6363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194362_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194362_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:44:47.01 +46:28:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.663 209612206687131136 086.19689831834 +46.47272458834 14.4861 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194409_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194409_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:53:58.33 +42:30:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.661 192386845210042624 088.49355776279 +42.50729470844 14.1038 13.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194415_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194415_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194420_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194420_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:07.53 +47:58:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194445_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194445_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:23.92 +43:12:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194490_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194490_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:03:02.88 +46:44:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194498_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194498_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:11.07 +42:46:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194502_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194502_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194508_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194508_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:38:38.05 +42:12:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194522_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194522_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194552_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194552_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:47.43 +45:58:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194563_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194563_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:21.55 +42:55:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.348 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194576_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194576_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194603_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194603_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194607_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194607_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194653_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194653_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194667_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194667_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194684_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194684_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:07.16 +48:23:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.177 210796720011848448 086.28058670363 +48.39677135116 14.7076 13.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194708_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194708_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194733_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194733_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:26.93 +41:55:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.794 194409843526240896 084.36191340515 +41.92779925005 14.5342 13.7011 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 194740_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194740_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194761_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194761_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194781_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194781_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194820_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194820_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:10.56 +47:17:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.519 210624925615467392 084.29384731994 +47.29912810693 14.6770 14.0165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194822_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194822_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194851_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194851_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:58.35 +43:11:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.984 196120580539087104 085.99325581244 +43.19690386859 14.7925 14.1596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194852_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194852_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:59:23.37 +47:47:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194853_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194853_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:10:00.32 +46:40:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.661 963408275991729408 092.50144899849 +46.67091546199 14.6329 14.0263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194863_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194863_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:04:02.17 +42:01:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194875_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194875_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194878_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194878_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:09.31 +42:01:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.050 192912854148386048 084.78895613482 +42.02448696040 14.5979 13.8298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194881_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194881_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194892_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194892_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194903_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194903_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194904_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194904_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194924_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194924_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:17.83 +49:03:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.616 211249448220215552 088.57374362350 +49.06165810540 14.5875 13.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194925_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194925_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 194933_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194933_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194943_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194943_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194946_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194946_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 194960_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194960_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:54:29.28 +41:58:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.211 192393682798261120 088.62226487653 +41.97986611135 14.6162 13.8330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194961_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194961_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:01:32.52 +48:06:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.351 969772008774566528 090.38550220391 +48.10359754765 14.5671 13.9081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194970_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 194970_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 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 194976_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 194976_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195008_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195008_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:21.59 +42:07:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.256 195916346254706304 084.83959266163 +42.12783046442 14.6530 13.8166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195013_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195013_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195017_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195017_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195044_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195044_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:14.41 +46:00:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.228 209520122588849024 084.30995072691 +46.00355328020 14.7209 14.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195061_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195061_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195066_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195066_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195068_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195068_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195072_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195072_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:35:36.99 +47:33:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.435 210828472705809408 083.90375351026 +47.56072668876 14.9023 14.3170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195073_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195073_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195084_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195084_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195088_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195088_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:37.06 +42:58:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.616 195976819393890048 085.65451684002 +42.97941518346 14.5822 13.6169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.616#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195090_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195090_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195102_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195102_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:06:20.34 +50:10:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.018 970420651915467392 091.58444291254 +50.17198110708 14.8015 14.1842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195104_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195104_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195110_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195110_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:34:45.09 +46:34:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.850 209042621006956416 083.68839796580 +46.57489993521 14.8767 14.4325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195111_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195111_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:42:45.56 +48:24:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.484 210974879549224704 085.69014813049 +48.41418871241 14.9400 14.2309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195121_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195121_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195127_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195127_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195128_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195128_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:09.44 +43:51:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.099 196341754174771072 086.28977359725 +43.85723911756 14.9162 14.3464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195132_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195132_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:39:14.04 +48:09:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.914 210886368864601472 084.80887747846 +48.16575509911 15.1527 14.4704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195135_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195135_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195146_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195146_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:19.60 +43:16:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.110 196232417190942464 085.33124361995 +43.27234679378 14.7302 13.8939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195148_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195148_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
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Considering the candidate 195152_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195152_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:41.13 +48:34:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.846 210816103199445760 086.42134714368 +48.57123440831 14.8715 14.3053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195154_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195154_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:00.40 +45:45:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.491 209496483088293888 084.25199752494 +45.76287179237 14.6601 13.9653 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195163_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195163_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:41:39.62 +44:11:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.732 197079870075095680 085.41533909835 +44.18824526463 14.8779 14.0108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195174_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195174_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195183_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195183_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195184_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195184_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195199_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195199_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195205_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195205_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:43:38.18 +42:37:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.342 193045658833000576 085.90892085682 +42.61971411691 14.8382 14.3556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195224_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195224_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:56:24.55 +44:09:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.127 193596548518439680 089.10212541234 +44.16590060267 14.6640 13.8937 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195230_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195230_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:50:13.56 +48:09:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.258 210344206553428736 087.55701002898 +48.16538563686 15.0530 14.4243 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195265_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195265_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:45:34.69 +42:48:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.641 193050778433822080 086.39458206188 +42.80942569474 14.8391 14.1472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195272_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195272_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:49:00.10 +44:11:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.132 196561072384805248 087.25102178615 +44.19548638207 14.9383 14.3963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195273_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195273_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195295_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 195295_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195354_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 195354_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:51:48.21 +42:33:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.071 193146603447491840 087.95104858750 +42.55210209705 14.7893 14.1703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
Preparing report for the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85273_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 85273_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:59:44.15 +47:37:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:57:24.14 +48:22:38.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 05:37:57.08 +44:41:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-15_22-31-24_20.00sec_-4.90C_LIGHT_0094 did not pass the final checks
**** FOUND 06:14:58.99 +46:47:46.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 6s
make_report_in_HTML.sh TOTAL: 223s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:27:32.41 +42:47:54.4
05:37:57.28 +43:37:31.0
05:47:53.20 +49:53:52.9
06:12:39.26 +50:06:40.3
05:51:27.83 +45:11:26.1
06:11:20.51 +47:33:11.0
05:51:21.70 +43:41:02.3
05:38:27.73 +43:02:32.1
05:50:46.63 +42:53:01.8
05:38:14.31 +42:37:03.1
05:45:52.58 +46:58:49.2
05:44:40.27 +43:25:24.7
06:21:13.41 +44:16:27.5
06:14:00.38 +49:18:12.6
05:55:17.38 +42:15:06.8
05:34:28.62 +48:41:18.0
06:00:16.25 +43:17:44.0
05:41:51.22 +42:23:27.2
06:25:14.44 +46:46:45.1
05:53:36.99 +50:13:44.9
05:35:07.27 +45:42:18.4
06:18:27.19 +43:47:22.9
05:43:43.17 +43:10:05.2
06:04:41.92 +42:52:10.0
06:26:29.59 +43:26:44.1
05:52:59.24 +46:57:29.8
06:29:25.06 +47:46:49.1
06:00:41.94 +42:25:35.9
06:13:19.13 +41:52:43.9
06:01:29.15 +48:45:21.1
06:21:31.86 +41:49:26.1
05:50:10.24 +43:38:47.0
06:19:41.80 +42:48:47.8
06:01:39.46 +45:44:14.4
05:37:56.69 +42:54:19.4
06:29:01.20 +41:59:52.8
05:49:29.01 +44:16:18.4
05:53:06.87 +44:56:00.4
05:43:47.28 +43:32:40.4
06:12:10.33 +50:14:53.6
06:13:43.55 +45:31:09.3
05:48:23.29 +49:46:56.8
05:37:16.44 +44:02:45.5
05:37:19.53 +44:51:37.2
05:39:19.09 +44:01:55.0
05:39:25.25 +42:39:19.0
05:37:52.55 +43:02:33.6
05:50:28.83 +44:11:33.7
05:49:06.60 +47:17:58.2
05:36:41.00 +50:02:55.8
05:45:50.41 +44:23:02.8
05:39:31.98 +44:38:40.6
06:26:29.82 +49:54:11.3
05:38:34.93 +44:30:50.6
06:00:34.89 +47:18:27.6
05:58:09.69 +48:37:11.6
05:37:13.19 +41:50:47.8
05:40:02.17 +45:53:53.9
05:58:41.88 +49:30:58.2
05:52:06.00 +42:43:08.4
05:55:10.42 +48:15:50.9
05:35:09.17 +46:30:55.8
05:51:08.02 +44:47:39.4
05:41:29.81 +42:17:20.4
05:42:53.10 +49:14:13.6
05:47:36.97 +45:17:23.8
05:41:58.24 +43:37:17.1
06:07:50.86 +49:44:53.1
05:52:24.36 +45:17:36.1
05:45:02.85 +41:57:31.1
05:56:24.40 +42:43:39.6
05:37:26.81 +41:45:27.6
05:48:36.31 +47:23:33.3
05:35:14.96 +48:10:55.0
05:40:39.05 +42:25:36.1
05:49:59.08 +42:16:50.5
05:53:21.72 +41:45:44.5
06:17:58.26 +47:16:16.1
05:37:22.86 +43:26:16.5
05:53:44.76 +44:22:32.8
05:52:38.15 +44:22:58.6
05:39:25.02 +45:28:18.3
05:42:50.03 +46:41:58.4
05:37:20.20 +44:24:55.6
05:47:17.08 +42:21:39.7
05:49:53.51 +47:39:01.5
05:37:55.81 +43:03:19.6
05:45:47.30 +49:40:08.3
05:37:12.27 +44:54:53.7
06:01:16.65 +46:03:25.7
05:43:08.19 +41:35:52.5
05:59:25.58 +46:37:18.2
05:38:26.15 +42:41:33.3
05:41:05.09 +41:35:04.2
05:54:33.63 +44:06:44.9
05:44:33.76 +44:04:36.6
########### Completed Aur-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:37:57.28 +43:37:31.0
05:47:53.20 +49:53:52.9
06:12:39.26 +50:06:40.3
05:51:27.83 +45:11:26.1
06:11:20.51 +47:33:11.0
05:51:21.70 +43:41:02.3
05:38:27.73 +43:02:32.1
05:50:46.63 +42:53:01.8
05:38:14.31 +42:37:03.1
05:45:52.58 +46:58:49.2
05:44:40.27 +43:25:24.7
06:21:13.41 +44:16:27.5
06:14:00.38 +49:18:12.6
05:55:17.38 +42:15:06.8
05:34:28.62 +48:41:18.0
06:00:16.25 +43:17:44.0
05:41:51.22 +42:23:27.2
06:25:14.44 +46:46:45.1
05:53:36.99 +50:13:44.9
05:35:07.27 +45:42:18.4
06:18:27.19 +43:47:22.9
05:43:43.17 +43:10:05.2
06:04:41.92 +42:52:10.0
06:26:29.59 +43:26:44.1
05:52:59.24 +46:57:29.8
06:29:25.06 +47:46:49.1
06:00:41.94 +42:25:35.9
06:13:19.13 +41:52:43.9
06:01:29.15 +48:45:21.1
06:21:31.86 +41:49:26.1
05:50:10.24 +43:38:47.0
06:19:41.80 +42:48:47.8
06:01:39.46 +45:44:14.4
05:37:56.69 +42:54:19.4
06:29:01.20 +41:59:52.8
05:49:29.01 +44:16:18.4
05:53:06.87 +44:56:00.4
05:43:47.28 +43:32:40.4
06:12:10.33 +50:14:53.6
06:13:43.55 +45:31:09.3
05:48:23.29 +49:46:56.8
05:37:16.44 +44:02:45.5
05:37:19.53 +44:51:37.2
05:39:19.09 +44:01:55.0
05:39:25.25 +42:39:19.0
05:37:52.55 +43:02:33.6
05:50:28.83 +44:11:33.7
05:49:06.60 +47:17:58.2
05:36:41.00 +50:02:55.8
05:45:50.41 +44:23:02.8
05:39:31.98 +44:38:40.6
06:26:29.82 +49:54:11.3
05:38:34.93 +44:30:50.6
06:00:34.89 +47:18:27.6
05:58:09.69 +48:37:11.6
05:37:13.19 +41:50:47.8
05:40:02.17 +45:53:53.9
05:58:41.88 +49:30:58.2
05:52:06.00 +42:43:08.4
05:55:10.42 +48:15:50.9
05:35:09.17 +46:30:55.8
05:51:08.02 +44:47:39.4
05:41:29.81 +42:17:20.4
05:42:53.10 +49:14:13.6
05:47:36.97 +45:17:23.8
05:41:58.24 +43:37:17.1
06:07:50.86 +49:44:53.1
05:52:24.36 +45:17:36.1
05:45:02.85 +41:57:31.1
05:56:24.40 +42:43:39.6
05:37:26.81 +41:45:27.6
05:48:36.31 +47:23:33.3
05:35:14.96 +48:10:55.0
05:40:39.05 +42:25:36.1
05:49:59.08 +42:16:50.5
05:53:21.72 +41:45:44.5
06:17:58.26 +47:16:16.1
05:37:22.86 +43:26:16.5
05:53:44.76 +44:22:32.8
05:52:38.15 +44:22:58.6
05:39:25.02 +45:28:18.3
05:42:50.03 +46:41:58.4
05:37:20.20 +44:24:55.6
05:47:17.08 +42:21:39.7
05:49:53.51 +47:39:01.5
05:37:55.81 +43:03:19.6
05:45:47.30 +49:40:08.3
05:37:12.27 +44:54:53.7
06:01:16.65 +46:03:25.7
05:43:08.19 +41:35:52.5
05:59:25.58 +46:37:18.2
05:38:26.15 +42:41:33.3
05:41:05.09 +41:35:04.2
05:54:33.63 +44:06:44.9
05:44:33.76 +44:04:36.6
06:27:32.41 +42:47:54.4
###################################################################################
05:37:57.28 +43:37:31.0 -- not an asteroid (will add it to exclusion list)
05:47:53.20 +49:53:52.9 -- not an asteroid (will add it to exclusion list)
06:12:39.26 +50:06:40.3 -- not an asteroid (will add it to exclusion list)
05:51:27.83 +45:11:26.1 -- not an asteroid (will add it to exclusion list)
06:11:20.51 +47:33:11.0 -- not an asteroid (will add it to exclusion list)
05:51:21.70 +43:41:02.3 -- not an asteroid (will add it to exclusion list)
05:38:27.73 +43:02:32.1 -- not an asteroid (will add it to exclusion list)
05:50:46.63 +42:53:01.8 -- not an asteroid (will add it to exclusion list)
05:38:14.31 +42:37:03.1 -- not an asteroid (will add it to exclusion list)
05:45:52.58 +46:58:49.2 -- not an asteroid (will add it to exclusion list)
05:44:40.27 +43:25:24.7 -- not an asteroid (will add it to exclusion list)
06:21:13.41 +44:16:27.5 -- not an asteroid (will add it to exclusion list)
06:14:00.38 +49:18:12.6 -- not an asteroid (will add it to exclusion list)
05:55:17.38 +42:15:06.8 -- not an asteroid (will add it to exclusion list)
05:34:28.62 +48:41:18.0 -- not an asteroid (will add it to exclusion list)
06:00:16.25 +43:17:44.0 -- not an asteroid (will add it to exclusion list)
05:41:51.22 +42:23:27.2 -- not an asteroid (will add it to exclusion list)
06:25:14.44 +46:46:45.1 -- not an asteroid (will add it to exclusion list)
05:53:36.99 +50:13:44.9 -- not an asteroid (will add it to exclusion list)
05:35:07.27 +45:42:18.4 -- not an asteroid (will add it to exclusion list)
06:18:27.19 +43:47:22.9 -- not an asteroid (will add it to exclusion list)
05:43:43.17 +43:10:05.2 -- not an asteroid (will add it to exclusion list)
06:04:41.92 +42:52:10.0 -- not an asteroid (will add it to exclusion list)
06:26:29.59 +43:26:44.1 -- not an asteroid (will add it to exclusion list)
05:52:59.24 +46:57:29.8 -- not an asteroid (will add it to exclusion list)
06:29:25.06 +47:46:49.1 -- not an asteroid (will add it to exclusion list)
06:00:41.94 +42:25:35.9 -- not an asteroid (will add it to exclusion list)
06:13:19.13 +41:52:43.9 -- not an asteroid (will add it to exclusion list)
06:01:29.15 +48:45:21.1 -- not an asteroid (will add it to exclusion list)
06:21:31.86 +41:49:26.1 -- not an asteroid (will add it to exclusion list)
05:50:10.24 +43:38:47.0 -- not an asteroid (will add it to exclusion list)
06:19:41.80 +42:48:47.8 -- not an asteroid (will add it to exclusion list)
06:01:39.46 +45:44:14.4 -- not an asteroid (will add it to exclusion list)
05:37:56.69 +42:54:19.4 -- not an asteroid (will add it to exclusion list)
06:29:01.20 +41:59:52.8 -- not an asteroid (will add it to exclusion list)
05:49:29.01 +44:16:18.4 -- not an asteroid (will add it to exclusion list)
05:53:06.87 +44:56:00.4 -- not an asteroid (will add it to exclusion list)
05:43:47.28 +43:32:40.4 -- not an asteroid (will add it to exclusion list)
06:12:10.33 +50:14:53.6 -- not an asteroid (will add it to exclusion list)
06:13:43.55 +45:31:09.3 -- not an asteroid (will add it to exclusion list)
05:48:23.29 +49:46:56.8 -- not an asteroid (will add it to exclusion list)
05:37:16.44 +44:02:45.5 -- not an asteroid (will add it to exclusion list)
05:37:19.53 +44:51:37.2 -- not an asteroid (will add it to exclusion list)
05:39:19.09 +44:01:55.0 -- not an asteroid (will add it to exclusion list)
05:39:25.25 +42:39:19.0 -- not an asteroid (will add it to exclusion list)
05:37:52.55 +43:02:33.6 -- not an asteroid (will add it to exclusion list)
05:50:28.83 +44:11:33.7 -- not an asteroid (will add it to exclusion list)
05:49:06.60 +47:17:58.2 -- not an asteroid (will add it to exclusion list)
05:36:41.00 +50:02:55.8 -- not an asteroid (will add it to exclusion list)
05:45:50.41 +44:23:02.8 -- not an asteroid (will add it to exclusion list)
05:39:31.98 +44:38:40.6 -- not an asteroid (will add it to exclusion list)
06:26:29.82 +49:54:11.3 -- not an asteroid (will add it to exclusion list)
05:38:34.93 +44:30:50.6 -- not an asteroid (will add it to exclusion list)
06:00:34.89 +47:18:27.6 -- not an asteroid (will add it to exclusion list)
05:58:09.69 +48:37:11.6 -- not an asteroid (will add it to exclusion list)
05:37:13.19 +41:50:47.8 -- not an asteroid (will add it to exclusion list)
05:40:02.17 +45:53:53.9 -- not an asteroid (will add it to exclusion list)
05:58:41.88 +49:30:58.2 -- not an asteroid (will add it to exclusion list)
05:52:06.00 +42:43:08.4 -- not an asteroid (will add it to exclusion list)
05:55:10.42 +48:15:50.9 -- not an asteroid (will add it to exclusion list)
05:35:09.17 +46:30:55.8 -- not an asteroid (will add it to exclusion list)
05:51:08.02 +44:47:39.4 -- not an asteroid (will add it to exclusion list)
05:41:29.81 +42:17:20.4 -- not an asteroid (will add it to exclusion list)
05:42:53.10 +49:14:13.6 -- not an asteroid (will add it to exclusion list)
05:47:36.97 +45:17:23.8 -- not an asteroid (will add it to exclusion list)
05:41:58.24 +43:37:17.1 -- not an asteroid (will add it to exclusion list)
06:07:50.86 +49:44:53.1 -- not an asteroid (will add it to exclusion list)
05:52:24.36 +45:17:36.1 -- not an asteroid (will add it to exclusion list)
05:45:02.85 +41:57:31.1 -- not an asteroid (will add it to exclusion list)
05:56:24.40 +42:43:39.6 -- not an asteroid (will add it to exclusion list)
05:37:26.81 +41:45:27.6 -- not an asteroid (will add it to exclusion list)
05:48:36.31 +47:23:33.3 -- not an asteroid (will add it to exclusion list)
05:35:14.96 +48:10:55.0 -- not an asteroid (will add it to exclusion list)
05:40:39.05 +42:25:36.1 -- not an asteroid (will add it to exclusion list)
05:49:59.08 +42:16:50.5 -- not an asteroid (will add it to exclusion list)
05:53:21.72 +41:45:44.5 -- not an asteroid (will add it to exclusion list)
06:17:58.26 +47:16:16.1 -- not an asteroid (will add it to exclusion list)
05:37:22.86 +43:26:16.5 -- not an asteroid (will add it to exclusion list)
05:53:44.76 +44:22:32.8 -- not an asteroid (will add it to exclusion list)
05:52:38.15 +44:22:58.6 -- not an asteroid (will add it to exclusion list)
05:39:25.02 +45:28:18.3 -- not an asteroid (will add it to exclusion list)
05:42:50.03 +46:41:58.4 -- not an asteroid (will add it to exclusion list)
05:37:20.20 +44:24:55.6 -- not an asteroid (will add it to exclusion list)
05:47:17.08 +42:21:39.7 -- not an asteroid (will add it to exclusion list)
05:49:53.51 +47:39:01.5 -- not an asteroid (will add it to exclusion list)
05:37:55.81 +43:03:19.6 -- not an asteroid (will add it to exclusion list)
05:45:47.30 +49:40:08.3 -- not an asteroid (will add it to exclusion list)
05:37:12.27 +44:54:53.7 -- not an asteroid (will add it to exclusion list)
06:01:16.65 +46:03:25.7 -- not an asteroid (will add it to exclusion list)
05:43:08.19 +41:35:52.5 -- not an asteroid (will add it to exclusion list)
05:59:25.58 +46:37:18.2 -- not an asteroid (will add it to exclusion list)
05:38:26.15 +42:41:33.3 -- not an asteroid (will add it to exclusion list)
05:41:05.09 +41:35:04.2 -- not an asteroid (will add it to exclusion list)
05:54:33.63 +44:06:44.9 -- not an asteroid (will add it to exclusion list)
05:44:33.76 +44:04:36.6 -- not an asteroid (will add it to exclusion list)
06:27:32.41 +42:47:54.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:34:28.62 +48:41:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:07.27 +45:42:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:09.17 +46:30:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:14.96 +48:10:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:41.00 +50:02:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:12.27 +44:54:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:13.19 +41:50:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.44 +44:02:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.53 +44:51:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:20.20 +44:24:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:22.86 +43:26:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:26.81 +41:45:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.55 +43:02:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:55.81 +43:03:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:56.69 +42:54:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:57.28 +43:37:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:14.31 +42:37:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:26.15 +42:41:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:27.73 +43:02:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:34.93 +44:30:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.09 +44:01:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:25.02 +45:28:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:25.25 +42:39:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:31.98 +44:38:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:02.17 +45:53:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:39.05 +42:25:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:05.09 +41:35:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:29.81 +42:17:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:51.22 +42:23:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:58.24 +43:37:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:50.03 +46:41:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:53.10 +49:14:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:08.19 +41:35:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:43.17 +43:10:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.28 +43:32:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:33.76 +44:04:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:40.27 +43:25:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:02.85 +41:57:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:47.30 +49:40:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.41 +44:23:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:52.58 +46:58:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:17.08 +42:21:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:36.97 +45:17:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:53.20 +49:53:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.29 +49:46:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:36.31 +47:23:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.60 +47:17:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:29.01 +44:16:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.51 +47:39:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:59.08 +42:16:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.24 +43:38:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.83 +44:11:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:46.63 +42:53:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:08.02 +44:47:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:21.70 +43:41:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:27.83 +45:11:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:06.00 +42:43:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:24.36 +45:17:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:38.15 +44:22:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:59.24 +46:57:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.87 +44:56:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:21.72 +41:45:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:36.99 +50:13:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:44.76 +44:22:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:33.63 +44:06:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.42 +48:15:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:17.38 +42:15:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:24.40 +42:43:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.69 +48:37:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:41.88 +49:30:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:25.58 +46:37:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:16.25 +43:17:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:34.89 +47:18:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:41.94 +42:25:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:16.65 +46:03:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:29.15 +48:45:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:39.46 +45:44:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:41.92 +42:52:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:50.86 +49:44:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:20.51 +47:33:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.33 +50:14:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:39.26 +50:06:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:19.13 +41:52:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:43.55 +45:31:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:00.38 +49:18:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:58.26 +47:16:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:27.19 +43:47:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:19:41.80 +42:48:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:13.41 +44:16:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.86 +41:49:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:14.44 +46:46:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.59 +43:26:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.82 +49:54:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:32.41 +42:47:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:01.20 +41:59:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:25.06 +47:46:49.1 -- 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)
05:34:28.62 +48:41:18.0 -- not a known variable star
05:35:07.27 +45:42:18.4 -- a known variable star
05:35:09.17 +46:30:55.8 -- not a known variable star
05:35:14.96 +48:10:55.0 -- not a known variable star
05:36:41.00 +50:02:55.8 -- not a known variable star
05:37:12.27 +44:54:53.7 -- not a known variable star
05:37:13.19 +41:50:47.8 -- not a known variable star
05:37:16.44 +44:02:45.5 -- not a known variable star
05:37:19.53 +44:51:37.2 -- not a known variable star
05:37:20.20 +44:24:55.6 -- not a known variable star
05:37:22.86 +43:26:16.5 -- not a known variable star
05:37:26.81 +41:45:27.6 -- not a known variable star
05:37:52.55 +43:02:33.6 -- not a known variable star
05:37:55.81 +43:03:19.6 -- not a known variable star
05:37:56.69 +42:54:19.4 -- a known variable star
05:37:57.28 +43:37:31.0 -- a known variable star
05:38:14.31 +42:37:03.1 -- not a known variable star
05:38:26.15 +42:41:33.3 -- not a known variable star
05:38:27.73 +43:02:32.1 -- not a known variable star
05:38:34.93 +44:30:50.6 -- not a known variable star
05:39:19.09 +44:01:55.0 -- not a known variable star
05:39:25.02 +45:28:18.3 -- not a known variable star
05:39:25.25 +42:39:19.0 -- not a known variable star
05:39:31.98 +44:38:40.6 -- not a known variable star
05:40:02.17 +45:53:53.9 -- not a known variable star
05:40:39.05 +42:25:36.1 -- a known variable star
05:41:05.09 +41:35:04.2 -- not a known variable star
05:41:29.81 +42:17:20.4 -- not a known variable star
05:41:51.22 +42:23:27.2 -- not a known variable star
05:41:58.24 +43:37:17.1 -- not a known variable star
05:42:50.03 +46:41:58.4 -- not a known variable star
05:42:53.10 +49:14:13.6 -- not a known variable star
05:43:08.19 +41:35:52.5 -- not a known variable star
05:43:43.17 +43:10:05.2 -- not a known variable star
05:43:47.28 +43:32:40.4 -- not a known variable star
05:44:33.76 +44:04:36.6 -- not a known variable star
05:44:40.27 +43:25:24.7 -- not a known variable star
05:45:02.85 +41:57:31.1 -- not a known variable star
05:45:47.30 +49:40:08.3 -- not a known variable star
05:45:50.41 +44:23:02.8 -- not a known variable star
05:45:52.58 +46:58:49.2 -- a known variable star
05:47:17.08 +42:21:39.7 -- not a known variable star
05:47:36.97 +45:17:23.8 -- not a known variable star
05:47:53.20 +49:53:52.9 -- not a known variable star
05:48:23.29 +49:46:56.8 -- not a known variable star
05:48:36.31 +47:23:33.3 -- not a known variable star
05:49:06.60 +47:17:58.2 -- not a known variable star
05:49:29.01 +44:16:18.4 -- not a known variable star
05:49:53.51 +47:39:01.5 -- a known variable star
05:49:59.08 +42:16:50.5 -- not a known variable star
05:50:10.24 +43:38:47.0 -- not a known variable star
05:50:28.83 +44:11:33.7 -- a known variable star
05:50:46.63 +42:53:01.8 -- not a known variable star
05:51:08.02 +44:47:39.4 -- not a known variable star
05:51:21.70 +43:41:02.3 -- not a known variable star
05:51:27.83 +45:11:26.1 -- a known variable star
05:52:06.00 +42:43:08.4 -- not a known variable star
05:52:24.36 +45:17:36.1 -- not a known variable star
05:52:38.15 +44:22:58.6 -- not a known variable star
05:52:59.24 +46:57:29.8 -- not a known variable star
05:53:06.87 +44:56:00.4 -- not a known variable star
05:53:21.72 +41:45:44.5 -- not a known variable star
05:53:36.99 +50:13:44.9 -- not a known variable star
05:53:44.76 +44:22:32.8 -- not a known variable star
05:54:33.63 +44:06:44.9 -- not a known variable star
05:55:10.42 +48:15:50.9 -- not a known variable star
05:55:17.38 +42:15:06.8 -- not a known variable star
05:56:24.40 +42:43:39.6 -- not a known variable star
05:58:09.69 +48:37:11.6 -- not a known variable star
05:58:41.88 +49:30:58.2 -- not a known variable star
05:59:25.58 +46:37:18.2 -- not a known variable star
06:00:16.25 +43:17:44.0 -- not a known variable star
06:00:34.89 +47:18:27.6 -- not a known variable star
06:00:41.94 +42:25:35.9 -- not a known variable star
06:01:16.65 +46:03:25.7 -- not a known variable star
06:01:29.15 +48:45:21.1 -- not a known variable star
06:01:39.46 +45:44:14.4 -- not a known variable star
06:04:41.92 +42:52:10.0 -- not a known variable star
06:07:50.86 +49:44:53.1 -- not a known variable star
06:11:20.51 +47:33:11.0 -- not a known variable star
06:12:10.33 +50:14:53.6 -- not a known variable star
06:12:39.26 +50:06:40.3 -- not a known variable star
06:13:19.13 +41:52:43.9 -- not a known variable star
06:13:43.55 +45:31:09.3 -- a known variable star
06:14:00.38 +49:18:12.6 -- not a known variable star
06:17:58.26 +47:16:16.1 -- not a known variable star
06:18:27.19 +43:47:22.9 -- not a known variable star
06:19:41.80 +42:48:47.8 -- not a known variable star
06:21:13.41 +44:16:27.5 -- not a known variable star
06:21:31.86 +41:49:26.1 -- not a known variable star
06:25:14.44 +46:46:45.1 -- a known variable star
06:26:29.59 +43:26:44.1 -- not a known variable star
06:26:29.82 +49:54:11.3 -- not a known variable star
06:27:32.41 +42:47:54.4 -- not a known variable star
06:29:01.20 +41:59:52.8 -- not a known variable star
06:29:25.06 +47:46:49.1 -- not a known variable star
Found 86 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
96 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 96 (excluding asteroids and hot pixels, 86 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461146.64639352 -observatory V36
00:08:03.38 -01:58:43.2 Mercury (0.0mag)
03:09:21.57 +17:54:45.5 Venus (-3.9mag)
00:18:15.40 +00:54:38.1 Mars (1.2mag)
07:12:41.82 +22:46:07.5 Jupiter (-2.1mag)
00:29:14.78 +00:49:23.3 Saturn (0.9mag)
03:47:43.66 +19:47:34.5 Uranus (5.8mag)
00:10:51.56 -00:15:15.0 Neptune (7.8mag)
20:33:45.65 -22:52:36.2 Pluto (14.5mag)
00:21:53.12 +04:45:38.3 Moon (-8.5mag)
-rw-r--r-- 1 apache apache 361 Apr 15 22:55 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461146.64639352:
07:12:43.95 +22:46:05.5 Io (5.8mag)
07:12:47.82 +22:45:57.2 Europa (5.9mag)
07:12:58.54 +22:45:28.5 Ganymede (5.4mag)
07:13:17.20 +22:44:55.0 Callisto (6.6mag)
07:16:01.68 +22:33:40.9 Himalia (15.3mag)
07:12:39.15 +22:46:11.6 Thebe (16.2mag)
07:16:13.25 +23:03:53.2 Elara (17.3mag)
07:11:35.31 +23:26:03.2 Pasiphae (17.4mag)
07:21:01.33 +22:44:09.6 Carme (18.5mag)
00:29:15.20 +00:49:49.6 Titan (8.8mag)
00:29:13.42 +00:49:27.2 Rhea (10.1mag)
00:28:54.55 +00:49:31.3 Iapetus (11.5mag)
00:29:22.58 +00:49:43.6 Hyperion (14.8mag)
00:30:51.57 +00:58:10.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 15 22:55 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.64639352:
15:39:08.06 -16:21:06.0 JWST
13:40:57.60 +55:21:34.6 Chandra
07:55:52.69 -36:16:53.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 15 22:55 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.64639352 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:03.83 -28:47:14.8 13.9mag P/2010 H2 (Vales)
05:06:50.36 -69:39:17.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:28.65 +31:26:18.2 17.2mag C/2017 K2 (PANSTARRS)
17:30:25.31 +10:33:54.1 17.6mag C/2021 G2 (ATLAS)
23:10:15.78 +29:14:04.7 17.1mag C/2022 E2 (ATLAS)
04:29:24.38 +26:02:32.8 16.0mag C/2022 N2 (PANSTARRS)
09:03:27.08 +32:01:07.0 16.2mag C/2022 QE78 (ATLAS)
08:31:05.72 -00:08:15.4 17.3mag C/2022 R6 (PANSTARRS)
18:53:41.84 +18:32:40.9 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:37.67 -11:31:10.0 17.5mag P/2023 B1 (PANSTARRS)
09:07:34.06 -11:51:35.0 17.6mag C/2023 F3 (ATLAS)
21:54:21.75 +62:54:53.3 17.5mag C/2023 H5 (Lemmon)
19:19:04.43 -03:44:05.6 14.1mag C/2023 R1 (PANSTARRS)
21:32:14.98 +85:55:53.7 17.8mag C/2023 X2 (Lemmon)
06:17:57.88 +63:30:44.6 17.2mag C/2024 A1 (ATLAS)
05:13:35.37 +18:21:25.6 11.1mag C/2024 E1 (Wierzchos)
16:19:10.98 +06:24:52.0 17.4mag C/2024 G6 (ATLAS)
20:20:51.19 +15:18:50.5 14.6mag C/2024 J3 (ATLAS)
03:26:29.96 -22:21:47.7 16.3mag C/2024 T5 (ATLAS)
05:16:50.16 +45:15:17.1 17.7mag C/2025 J1 (Borisov)
13:38:13.72 +45:35:10.4 15.2mag C/2025 L1 (ATLAS)
03:25:30.32 -26:14:04.4 17.8mag C/2025 Q3 (ATLAS)
23:44:42.09 +18:33:47.2 8.5mag C/2025 R3 (PANSTARRS)
12:54:03.32 +03:01:18.2 17.4mag C/2025 Y1 (ATLAS)
03:29:08.21 +02:36:15.8 13.3mag C/2026 A1 (MAPS)
23:59:59.70 +37:14:47.1 14.6mag C/2026 B2 (Sun-Gao)
18:43:13.24 -09:42:40.4 11.8mag 10P/Tempel
15:00:06.66 +03:11:38.9 14.0mag 24P/Schaumasse
11:02:45.81 -01:31:17.2 15.7mag 29P/Schwassmann-Wachmann
18:01:00.38 -09:36:16.9 17.9mag 40P/Vaisala
10:37:33.51 -04:05:14.0 16.9mag 43P/Wolf-Harrington
01:48:53.96 +17:30:45.4 17.2mag 47P/Ashbrook-Jackson
07:11:02.01 +36:58:53.6 17.0mag 63P/Wild
23:29:14.62 -11:25:59.6 15.7mag 65P/Gunn
04:03:38.33 +21:18:19.9 15.9mag 76P/West-Kohoutek-Ikemura
01:05:53.85 +08:15:27.0 14.3mag 78P/Gehrels
23:03:26.78 -09:20:52.2 14.6mag 88P/Howell
02:10:48.78 +20:40:53.3 15.1mag 93P/Lovas
04:55:04.68 +32:17:44.5 16.2mag 123P/West-Hartley
08:28:32.03 +38:17:37.7 16.2mag 124P/Mrkos
02:33:26.47 +14:23:10.9 16.4mag 128P/Shoemaker-Holt
02:47:49.41 +14:30:40.0 17.5mag 131P/Mueller
01:26:55.94 +13:17:21.4 10.6mag 141P/Machholz
01:35:50.48 +04:55:43.5 10.6mag 141P-A/Machholz
00:21:03.93 +00:49:57.5 12.8mag 141P-D/Machholz
02:06:10.95 +06:41:16.4 17.8mag 141P-I/Machholz
01:02:47.13 -01:27:07.8 15.1mag 162P/SidingSpring
14:51:10.51 -00:03:10.2 17.7mag 210P/Christensen
21:39:16.21 -11:24:47.6 17.6mag 218P/LINEAR
17:16:36.35 -13:54:56.2 16.1mag 235P/LINEAR
05:34:47.85 +34:42:36.5 16.8mag 240P/NEAT
07:38:33.91 -05:09:04.6 17.7mag 242P/Spahr
22:17:16.42 -20:56:27.9 17.9mag 260P/McNaught
01:58:29.22 +20:29:51.1 18.0mag 295P/LINEAR
15:42:35.40 +07:00:00.7 17.5mag 391P/Kowalski
07:34:15.10 +21:21:59.6 17.7mag 450P/LONEOS
05:36:05.01 +45:01:27.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 15 22:55 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 15 22:55 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:52:32.558 +54:28:28.21 AT 2026iyo 2026-04-07.50 19.8736
12:10:51.131 -15:24:05.80 AT 2026iyn 2026-04-07.49 19.8
10:03:32.464 +00:47:38.92 AT 2026iym 2026-04-09.07 21.7842
09:57:46.577 +02:32:54.17 AT 2026iyl 2026-04-09.07 21.1159
12:09:21.288 -14:20:40.69 AT 2026iyk 2026-02-24.42 19.0617
11:32:15.323 +26:34:23.97 AT 2026iyi 2026-04-07.27 20.0038
08:41:36.643 +41:14:51.53 AT 2026iyh 2026-03-18.28 20.5874
11:10:47.748 -02:27:00.61 AT 2026iyg 2026-04-07.26 20.12
11:41:25.329 -11:32:16.55 AT 2026iyf 2026-04-07.25 20.8489
09:58:35.594 -17:44:37.57 AT 2026iye 2026-04-08.19 19.4848
07:48:08.582 +43:35:35.35 AT 2026iyd 2026-04-05.16 19.8382
11:13:43.729 +21:50:31.84 AT 2026iyc 2026-04-05.18 20.0005
08:02:45.458 +40:40:22.73 AT 2026iyb 2026-03-26.18 20.4831
13:05:52.496 +64:22:32.75 AT 2026iya 2026-03-08.94 19.29
05:15:26.423 -02:54:24.54 AT 2026ixz 2026-04-08.14 19.1905
14:04:24.118 +43:40:15.80 AT 2026ixt 2026-04-08.93 19.74
13:12:41.279 +38:05:24.08 AT 2026ixs 2026-04-08.93 20.18
13:21:56.843 -04:01:33.33 AT 2026ixr 2026-04-08.90 19.48
12:04:52.343 +69:44:57.80 AT 2026ixq 2026-04-08.89 19.03
21:31:46.671 +04:33:36.35 AT 2026ixp 2026-04-08.51 19.1697
-rw-r--r-- 1 apache apache 30K Apr 15 22:55 tns_transients_list.txt
