This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG
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
target,2461140.6808,13.81,0.05,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 20260410.1808 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 J090.2681+43.7611,2461140.6808,13.77,0.05,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
ATO J090.2681+43.7611 20260410.1808 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 J086.5752+41.8092,2461140.6808,13.72,0.05,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 J086.5752+41.8092 20260410.1808 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,2461140.6808,13.79,0.05,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 20260410.1808 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 J085.4195+46.7700,2461140.6808,13.71,0.05,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
ATO J085.4195+46.7700 20260410.1808 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.7424+43.7797,2461140.6808,13.72,0.05,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 J084.7424+43.7797 20260410.1808 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 J085.6618+45.4525,2461140.6808,13.75,0.05,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 J085.6618+45.4525 20260410.1808 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.63,0.05,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
target 20260410.1808 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.59,0.05,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
target 20260410.1808 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 J087.8530+42.8735,2461140.6808,13.41,0.05,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
ATO J087.8530+42.8735 20260410.1808 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,2461140.6808,13.60,0.05,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 20260410.1808 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.39,0.05,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 20260410.1808 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.2533+41.9469,2461140.6808,13.23,0.05,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 J086.2533+41.9469 20260410.1808 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197668173218550912,2461140.6808,13.36,0.05,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 197668173218550912 20260410.1808 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.12,0.05,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 20260410.1808 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.4002+44.3284,2461140.6808,13.12,0.05,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 J090.4002+44.3284 20260410.1808 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.1267+46.2073,2461140.6808,13.17,0.05,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 J085.1267+46.2073 20260410.1808 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196183179687428352,2461140.6808,13.41,0.05,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 196183179687428352 20260410.1808 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2220+45.5909,2461140.6808,13.30,0.05,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 J087.2220+45.5909 20260410.1808 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.1681+42.8723,2461140.6808,13.03,0.05,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 20260410.1808 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461140.6808,13.17,0.05,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
Gaia DR3 197994904265884544 20260410.1808 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461140.6808,13.09,0.05,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 20260410.1808 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.9718+42.7833,2461140.6808,12.82,0.05,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 J096.9718+42.7833 20260410.1808 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,12.73,0.05,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 20260410.1808 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3290+41.8878,2461140.6808,12.87,0.05,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
ATO J093.3290+41.8878 20260410.1808 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,12.66,0.05,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 20260410.1808 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192765386447163520,2461140.6808,12.77,0.05,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
Gaia DR3 192765386447163520 20260410.1808 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8200+43.1870,2461140.6808,12.54,0.05,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
ATO J096.8200+43.1870 20260410.1808 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 192293833399060608,2461140.6808,12.62,0.05,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
Gaia DR3 192293833399060608 20260410.1808 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5437+43.6538,2461140.6808,12.64,0.05,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 20260410.1808 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 959099633519521408,2461140.6808,11.62,0.05,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
Gaia DR3 959099633519521408 20260410.1808 11.62CV 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 192332281946145280,2461140.6808,11.43,0.05,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
Gaia DR3 192332281946145280 20260410.1808 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197617561323923456,2461140.6808,11.16,0.05,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
Gaia DR3 197617561323923456 20260410.1808 11.16CV 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 J095.2458+42.5740,2461140.6808,10.63,0.05,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
ATO J095.2458+42.5740 20260410.1808 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192716728762870272,2461140.6808,11.54,0.05,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
Gaia DR3 192716728762870272 20260410.1808 11.54CV 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 196564783236506368,2461140.6808,11.74,0.05,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 20260410.1808 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196796848908972032,2461140.6808,12.35,0.05,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
Gaia DR3 196796848908972032 20260410.1808 12.35CV 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 197992945761095424,2461140.6808,12.79,0.05,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 197992945761095424 20260410.1808 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 J090.6351+48.1884,2461140.6808,12.89,0.05,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
ATO J090.6351+48.1884 20260410.1808 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,12.96,0.05,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 20260410.1808 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4626+44.3866,2461140.6808,13.13,0.05,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 20260410.1808 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 208219778289730304,2461140.6808,13.11,0.05,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 208219778289730304 20260410.1808 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1509+45.4814,2461140.6808,13.04,0.05,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 J089.1509+45.4814 20260410.1808 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.12,0.05,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 20260410.1808 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461140.6808,13.01,0.05,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
ATO J084.3195+44.0466 20260410.1808 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.06,0.05,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 20260410.1808 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.12,0.05,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 20260410.1808 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 193210860455981696,2461140.6808,13.25,0.05,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 193210860455981696 20260410.1808 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.05,0.05,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 20260410.1808 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 J084.8541+42.6555,2461140.6808,13.33,0.05,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
ATO J084.8541+42.6555 20260410.1808 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 J087.3152+41.9461,2461140.6808,13.36,0.05,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 J087.3152+41.9461 20260410.1808 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.8798+49.8178,2461140.6808,13.30,0.05,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 J084.8798+49.8178 20260410.1808 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5381+48.6224,2461140.6808,13.31,0.05,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
ATO J089.5381+48.6224 20260410.1808 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,2461140.6808,13.32,0.05,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 20260410.1808 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210103654024515072,2461140.6808,13.48,0.05,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 210103654024515072 20260410.1808 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2615+46.3117,2461140.6808,13.36,0.05,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 J088.2615+46.3117 20260410.1808 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461140.6808,13.38,0.05,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 J087.2776+47.3006 20260410.1808 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 J089.6159+43.7708,2461140.6808,13.60,0.05,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 J089.6159+43.7708 20260410.1808 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.69,0.05,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 20260410.1808 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210091314583157888,2461140.6808,13.64,0.05,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 210091314583157888 20260410.1808 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.69,0.05,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 20260410.1808 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963235824465355264,2461140.6808,13.39,0.05,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 963235824465355264 20260410.1808 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196376556292031232,2461140.6808,13.69,0.05,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
Gaia DR3 196376556292031232 20260410.1808 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,13.61,0.05,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
target 20260410.1808 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 969647312987085056,2461140.6808,13.62,0.05,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
Gaia DR3 969647312987085056 20260410.1808 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.0035+48.1617,2461140.6808,13.74,0.05,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 J092.0035+48.1617 20260410.1808 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.1521+44.2433,2461140.6808,13.92,0.05,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 J086.1521+44.2433 20260410.1808 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193139186041201280,2461140.6808,13.83,0.05,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
Gaia DR3 193139186041201280 20260410.1808 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 J090.7392+43.2693,2461140.6808,13.81,0.05,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
ATO J090.7392+43.2693 20260410.1808 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 198055613627966848,2461140.6808,13.88,0.05,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 198055613627966848 20260410.1808 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
Gaia DR3 961508762277910144,2461140.6808,13.96,0.05,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
Gaia DR3 961508762277910144 20260410.1808 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
ATO J088.6179+43.5583,2461140.6808,13.71,0.05,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
ATO J088.6179+43.5583 20260410.1808 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195947132580142080,2461140.6808,13.78,0.05,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 20260410.1808 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053730.29+442702.5,2461140.6808,13.79,0.05,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
ASASSN-V J053730.29+442702.5 20260410.1808 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 J088.1029+43.5925,2461140.6808,13.96,0.05,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 J088.1029+43.5925 20260410.1808 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
ATO J083.9689+44.1503,2461140.6808,14.06,0.05,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 J083.9689+44.1503 20260410.1808 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6808,14.01,0.05,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
target 20260410.1808 14.01CV 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 196584363989884800,2461140.6808,13.78,0.05,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 196584363989884800 20260410.1808 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2431+43.3380,2461140.6808,13.99,0.05,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
ATO J088.2431+43.3380 20260410.1808 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8783+42.8003,2461140.6808,10.56,0.05,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
ATO J096.8783+42.8003 20260410.1808 10.56CV 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
## 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: 2461140.68108601 10.04.2026 04:20:35.831 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
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: 10 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): 16370
Objects passed selection criteria: 16341
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 14530.8
Average stars matched: 14166.5 (97.4932 %)
Memory usage VmPeak: 122832 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 23:36:51 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: 2461140.68108601 10.04.2026 04:20:35.831 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 330
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: 78 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): 124898
Objects passed selection criteria: 124555
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: 113281
Average stars matched: 109344 (96.5241 %)
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 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 23:39:14 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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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: 2461140.68048054
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# 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 06:00:10.090 +45:57:04.52
Angular distance between the image centers 0.0872 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:12.833 +45:57:07.25
Angular distance between the image centers 0.0927 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 06:00:10.090 +45:57:04.52
Second-epoch second image center 06:00:12.833 +45:57:07.25
Angular distance between the image centers 0.00798 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.P1vgUbmHaw
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.Nz4tVirM6j
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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits &> /tmp/tmp.ICyz2lPGkG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits &> /tmp/tmp.hruE3bZ7A4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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 9 candidate transients before the final filtering. (Hard limit: 3000)
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
2.7 pix fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
2.7 pix fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
All-image limiting magnitude estimate: 14.9 (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.P1vgUbmHaw (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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.Nz4tVirM6j (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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.ICyz2lPGkG (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1213, passed=17545
Got 17545 stars (including 16320 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 17545 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 40.1 to 51.2)
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(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 17138 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 40.1 to 51.2)
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(), 17139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 17139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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.hruE3bZ7A4 (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1197, passed=17466
Got 17466 stars (including 16251 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 17466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 51.2)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 17134 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 51.2)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 17131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 17131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31385.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31049_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31049_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:27.55 +42:19:24.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31163_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31163_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:28.48 +43:00:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31166_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31166_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:59:43.44 +44:59:09.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31181_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31181_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:14:59.00 +46:47:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31192_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31192_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:22.93 +46:49:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31296_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31296_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:45:42.89 +43:37:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31375_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31375_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:04:29.88 +43:09:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.903 961254401433213440 091.12410745222 +43.15702779599 12.3767 11.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31381_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31381_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:05:57.46 +43:47:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.750 961201758017019648 091.48936574688 +43.78965603324 12.2410 11.5458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31385_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 31385_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:14:23.66 +46:49:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.895 968668648856984832 093.59826702611 +46.82539996683 12.0731 11.3523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# 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 06:00:10.090 +45:57:04.52
Angular distance between the image centers 0.0872 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:12.833 +45:57:07.25
Angular distance between the image centers 0.0927 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 06:00:10.090 +45:57:04.52
Second-epoch second image center 06:00:12.833 +45:57:07.25
Angular distance between the image centers 0.00798 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.kQ7DJS4vjq
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.S5llmXoFow
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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits &> /tmp/tmp.tQyBELOiy3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits &> /tmp/tmp.x51LV6WY9f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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 256 candidate transients before the final filtering. (Hard limit: 3000)
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
2.2 pix fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
14.1 mag. fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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.kQ7DJS4vjq (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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.S5llmXoFow (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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.tQyBELOiy3 (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=12209, passed=124514
Got 124514 stars (including 112188 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 124514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 40.1 to 51.2)
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: 938 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 122396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 40.1 to 51.2)
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: 938 matched stars entering correct_measured_positions(), 122397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 122397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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.x51LV6WY9f (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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=12029, passed=123806
Got 123806 stars (including 111662 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 123806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 40.1 to 51.2)
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: 935 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 121599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 40.1 to 51.2)
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: 935 matched stars entering correct_measured_positions(), 121598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 121599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/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_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-19-43_20.00sec_-5.00C_LIGHT_0058.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.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_2026-04-09_CI_Aur-02-Q2b1x1_232453_TTUQ2b1x1_30432_sXUiW1UG/wcs_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out192141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out143438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192346.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__out192363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195070.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 119s
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: 53s
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Considering the candidate 192136_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192136_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192141_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192141_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:06.90 +44:51:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.332 196828219350531840 087.27927115291 +44.85760481161 14.7437 14.1831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192151_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192151_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:55:24.94 +44:41:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.640 196635151980646144 088.85414613525 +44.68995979904 14.5307 13.7359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192154_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192154_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:52:56.59 +47:14:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.878 198016619620483712 088.23614600639 +47.23587292125 14.7025 14.1467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192170_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192170_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:25.32 +43:52:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.995 196494345772948224 087.35588359387 +43.87764212422 14.6734 14.0072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192176_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192176_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192181_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192181_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192183_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192183_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:55:50.62 +46:34:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.918 197820666033064960 088.96126035058 +46.58298492236 14.7448 14.2444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192186_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192186_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:26.24 +41:33:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.892 192660692324627584 085.60946313896 +41.56597808933 14.4317 13.7747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192189_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192189_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192193_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192193_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:28.15 +46:16:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.416 209550187359249280 085.11742079075 +46.27087097741 14.4673 13.8137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192195_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192195_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192198_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192198_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:04.88 +46:58:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.504 197994865611149056 088.27091123366 +46.96733450096 14.7114 13.9657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192199_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192199_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192200_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192200_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:13.46 +48:11:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.130 210875511187223424 085.05655203201 +48.19186304855 14.5905 14.1514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192201_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192201_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:51:26.72 +46:46:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.647 197986108172957696 087.86157153688 +46.76843644372 14.5768 13.9510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192202_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192202_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:01.44 +43:40:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 0.328 197050694359020544 084.25598611668 +43.68163173446 14.4297 13.5493 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 192204_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192204_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192205_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192205_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192215_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192215_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:35:12.69 +44:57:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192217_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192217_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:01:01.96 +48:38:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.402 969814580490083584 090.25833473206 +48.64796014011 14.3056 13.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192229_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192229_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192236_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192236_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 192238_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192238_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:57.71 +42:35:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192244_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192244_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192255_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192255_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:29:38.02 +44:18:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.011 964992259930024448 097.40763813683 +44.31076371524 13.8772 13.3504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192260_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192260_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:14:39.85 +44:54:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.150 962443145300331008 093.66577241718 +44.91289522274 14.2723 13.6786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192268_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192268_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192271_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192271_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:31.64 +44:52:41.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 192273_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192273_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:26.81 +43:07:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192280_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192280_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192282_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192282_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:02.67 +45:28:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.375 197434806172188416 085.26166733685 +45.47032738571 14.3016 13.7120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192283_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192283_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192289_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192289_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:20.14 +41:55:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.030 193092800394897280 087.33390194821 +41.92263064796 14.2183 13.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192290_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192290_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:09.21 +45:22:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.750 196739021469243136 089.28834194525 +45.38023735729 13.9714 13.3170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192291_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192291_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 192295_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192295_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:46:52.35 +41:48:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192299_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192299_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192300_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192300_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192305_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192305_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192317_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192317_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192318_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192318_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:31.83 +44:07:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.441 197112614905505664 084.63250258375 +44.11974810978 13.9174 13.3239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192319_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192319_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:28:39.62 +42:43:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.220 958799810442205952 097.16440234056 +42.73155528775 13.7438 12.9800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192324_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192324_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192325_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192325_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:28.87 +46:52:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.401 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192326_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192326_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:50:32.96 +42:15:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192328_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192328_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192333_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192333_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192338_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192338_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192339_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192339_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:46.55 +47:09:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192346_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192346_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192350_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192350_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:45.65 +44:06:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192352_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192352_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192353_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192353_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:53.96 +47:59:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192354_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192354_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:30.27 +43:50:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.179 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192358_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192358_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192359_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192359_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:29:25.72 +47:46:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.431 967453825946335488 097.35734066624 +47.78321996652 13.4630 12.7527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192361_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192361_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:56:29.61 +45:53:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.836 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192363_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192363_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192365_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192365_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192366_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192366_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:49.53 +41:27:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.399 191392199503897728 084.20686554759 +41.46595927300 13.6795 13.3475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192369_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192369_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:16:36.28 +44:32:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.660 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192370_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192370_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:11.27 +43:24:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192383_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192383_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 192384_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192384_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:19:25.24 +44:38:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.097 962202214814317312 094.85547961849 +44.64084749790 13.1782 12.5035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192389_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192389_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:50:43.05 +46:13:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.902 197888973193024896 087.68013303510 +46.21714659712 13.2634 12.3569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192390_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192390_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:24.24 +42:05:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192391_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192391_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:31:06.95 +48:10:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192393_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192393_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:01.68 +46:28:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192394_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192394_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:46.16 +43:18:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192398_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192398_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:57.64 +44:20:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.408 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192399_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192399_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:13.70 +44:08:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192401_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192401_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:17.33 +42:28:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192404_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192404_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192405_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192405_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:23.49 +49:53:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192407_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192407_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:19:45.81 +41:47:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 1.146 960005493662278016 094.94078123081 +41.78814390889 12.2757 11.8217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192408_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192408_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:51:38.17 +48:20:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192409_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192409_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:54:42.23 +43:39:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.692 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192410_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192410_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192411_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192411_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:55.65 +42:54:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)GAIADR2_OUTPUT=# 4.405 196195961507760768 084.48025002876 +42.90529955301 12.0708 11.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192412_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192412_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:45.93 +43:34:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192413_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192413_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:09.08 +46:13:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192414_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192414_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192415_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192415_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:56:09.63 +44:18:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192417_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192417_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192420_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192420_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:27.55 +42:19:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192536_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192536_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:28.50 +43:00:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192556_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192556_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:22.92 +46:49:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192695_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192695_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192749_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192749_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:19.53 +42:40:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192823_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192823_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:46:26.51 +47:55:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192826_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192826_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:51:47.65 +48:44:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192864_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192864_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 192962_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 192962_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:17.80 +45:03:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192994_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 192994_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193020_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193020_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:03.07 +42:12:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193055_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193055_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:07.65 +44:53:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193056_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193056_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:02.78 +50:02:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193128_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193128_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:51:18.26 +46:14:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193140_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193140_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:05:50.19 +44:39:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193168_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193168_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:34:37.53 +45:55:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193184_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193184_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:48:45.98 +46:35:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193204_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193204_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:48:04.13 +43:19:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193220_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193220_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:16.78 +47:26:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.427 210685257018537344 085.32032670455 +47.44841135014 13.1638 12.3736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193228_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193228_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:43.13 +48:20:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193232_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193232_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:25.91 +48:47:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193242_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193242_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:03:13.62 +42:56:26.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193277_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193277_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:52.78 +47:06:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193320_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193320_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:47:45.37 +50:03:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193327_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193327_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:46.09 +45:53:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193330_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193330_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:32.63 +43:42:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193340_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193340_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193381_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193381_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:11.97 +45:24:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193468_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193468_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:01:04.70 +50:00:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193478_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193478_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:46.31 +43:03:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193496_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193496_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:44.74 +44:40:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.012 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193499_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193499_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:11:00.98 +47:29:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193507_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193507_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:14.26 +50:00:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193508_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193508_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:32.72 +41:57:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193519_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193519_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:46.47 +46:04:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193566_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193566_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:06.52 +44:51:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193570_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193570_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:35:35.24 +44:15:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193595_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193595_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:24.36 +42:59:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193638_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193638_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193659_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193659_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:34:02.55 +46:44:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193661_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193661_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:22.11 +42:59:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193682_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193682_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:50.78 +48:07:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.257 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193687_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193687_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 193695_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193695_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:14.64 +43:32:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193704_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193704_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:52:03.70 +49:32:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193715_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193715_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:00:14.04 +47:43:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193727_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193727_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:31.08 +44:15:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.211 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 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 193743_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193743_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193747_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193747_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:28.26 +42:14:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193750_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193750_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193751_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193751_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:48:23.32 +49:46:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 0.660 211485637061247744 087.09740055049 +49.78256265660 13.8223 13.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193752_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193752_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 193756_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193756_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:50.43 +49:49:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193768_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193768_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:28.47 +42:00:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.807 195912429244634624 084.36928975315 +42.01213215946 13.8357 13.3198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193782_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193782_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:18.53 +44:01:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193798_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193798_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:23.49 +49:49:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 0.434 214254619657430144 084.84769115489 +49.82477197399 14.0502 13.3596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193813_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193813_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:44:39.67 +43:57:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193873_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193873_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:27.93 +47:51:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.864 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193882_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193882_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193888_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193888_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193891_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193891_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:44.65 +42:36:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.212 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193896_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193896_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:24.84 +49:14:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.108 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193897_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193897_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:51:18.86 +43:17:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.178 193427528667708288 087.82879815788 +43.29576806055 13.9092 13.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193935_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193935_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:18.65 +47:12:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.648 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193942_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193942_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:46:39.76 +43:21:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.591 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193944_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193944_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:48:44.80 +49:34:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.549 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 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 193963_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193963_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193974_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193974_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193983_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 193983_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 193984_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193984_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:25.47 +42:20:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.581 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193987_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193987_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:15.63 +45:20:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193991_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 193991_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:03:21.32 +42:41:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.062 960875035561541376 090.83923379420 +42.69689639166 13.9565 13.4004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194006_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194006_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:16.22 +43:16:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194011_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194011_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194016_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194016_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194034_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194034_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:57.48 +42:25:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194058_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194058_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:46:32.88 +45:16:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.829 197288708563260416 086.63729611406 +45.26823510755 14.1987 13.5727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194062_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194062_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:59.53 +46:21:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194079_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194079_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:35:30.86 +48:04:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194082_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194082_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:08:19.27 +41:46:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194090_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194090_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:50:06.36 +46:08:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194098_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194098_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:36:07.14 +47:47:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.899 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194112_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194112_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:45:24.69 +43:50:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194116_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194116_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:25:45.48 +45:22:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194119_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194119_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194123_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194123_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:50:24.01 +41:41:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194142_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194142_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:11:51.70 +45:03:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.691 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194146_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194146_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194156_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194156_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:02.59 +46:20:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.149 209551767907386496 085.26048581597 +46.34391398611 14.2046 13.6286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194162_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194162_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:59.86 +47:35:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.912 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194217_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194217_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:54:37.45 +42:21:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.423 192463089469495040 088.65657575832 +42.35446354390 14.1602 13.5191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194231_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194231_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194233_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194233_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194251_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194251_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194259_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194259_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:53:58.37 +42:30:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.126 192386845210042624 088.49355776279 +42.50729470844 14.1038 13.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194284_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194284_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:04:15.56 +46:54:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.656 963649000318538496 091.06438493489 +46.91042639042 14.3324 13.7065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194318_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194318_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194324_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194324_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194352_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194352_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:07.33 +47:58:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194362_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194362_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:54:21.54 +42:55:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.136 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:15.64 +45:41:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.337 197673194035728768 087.31572492044 +45.68826913353 14.3025 13.6695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194383_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194383_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194399_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194399_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194402_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194402_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194412_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194412_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:12:20.06 +50:12:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194468_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194468_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194564_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194564_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:34:26.99 +46:08:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.752 208267160368960000 083.61303104489 +46.14235709444 14.3490 13.4590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194565_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194565_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194567_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194567_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:34.83 +44:30:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.451 197324992449032448 084.64566956412 +44.51452500122 14.4798 13.9246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194583_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194583_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:47:45.92 +45:04:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.143 197224455852769280 086.94120466206 +45.08119300612 14.6628 13.9871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194591_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194591_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:00:27.40 +42:54:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.562 960919050386214528 090.11419266104 +42.91073825498 14.5959 13.7863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194604_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194604_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194607_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194607_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:45:03.83 +49:39:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.687 214110446194930560 086.26624730253 +49.65684395412 14.4453 13.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194642_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:23.02 +44:38:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194652_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194652_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:54:16.18 +41:58:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.802 192299846352802176 088.56714256474 +41.96732700967 14.4620 13.6806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194658_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194658_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194668_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194668_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194683_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194683_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:13.56 +44:55:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.128 196664632636062336 089.30690131675 +44.92317349648 14.3868 13.6231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194700_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194700_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194702_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194702_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194756_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194756_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:54:17.72 +49:03:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.385 211249448220215552 088.57374362350 +49.06165810540 14.5875 13.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194761_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194761_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194775_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194775_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194783_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194783_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194799_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194799_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:31.49 +41:47:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.722 192857917222804096 085.63183763419 +41.79599060573 14.3975 13.5331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194843_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194843_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:14.26 +46:00:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.371 209520122588849024 084.30995072691 +46.00355328020 14.7209 14.1388 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 194869_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194869_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194882_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194882_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:56:24.35 +44:09:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.806 193596548518439680 089.10212541234 +44.16590060267 14.6640 13.8937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194901_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194901_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:01:32.48 +48:06:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.218 969772008774566528 090.38550220391 +48.10359754765 14.5671 13.9081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194903_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194903_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:46:50.76 +46:54:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.378 209674981928902528 086.71240249685 +46.91581834305 14.7890 14.1581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194918_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194918_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194924_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194924_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:42:52.99 +49:14:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.341 211070330903780864 085.72132629808 +49.23734255589 14.8139 14.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194926_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194926_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:40:09.07 +43:18:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.746 196241664257129856 085.03844580851 +43.30109303773 14.5371 13.7195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194932_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194932_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:34.41 +42:20:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.653 195935209751002752 084.89360411427 +42.33684241881 14.4030 13.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194937_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194937_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194941_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194941_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194944_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194944_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:49:29.12 +42:28:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.156 193169113373091712 087.37164333181 +42.46913586159 14.6077 13.7720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194948_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194948_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:52:30.15 +48:24:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.181 210329809822920832 088.12611379132 +48.40300750766 14.8966 13.9573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194950_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194950_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:41:38.56 +44:06:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.633 197078667484262784 085.41079470783 +44.11501107746 14.8953 14.0313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194951_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194951_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194959_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194959_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:47:47.75 +46:06:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.296 197898903157488896 086.94945708024 +46.10046081619 14.7625 14.0259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194967_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194967_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:44:45.80 +46:15:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.613 209594442702454912 086.19143349104 +46.25408139692 14.8781 14.2413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194968_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194968_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:35.00 +47:30:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.245 210650661059367936 084.64650828332 +47.50588003746 14.8314 14.4324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194971_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194971_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 194981_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 194981_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194988_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194988_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:34:39.28 +46:05:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.554 208265889058644224 083.66428865771 +46.09368319815 14.6618 13.8228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194992_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194992_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:50:20.51 +43:16:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.394 193453062250916736 087.58557619485 +43.27534854733 14.9372 14.3156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194996_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194996_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:56:39.24 +47:38:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.702 198121691700621312 089.16352636068 +47.63575037231 15.0134 14.4237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194998_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 194998_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:45:41.00 +48:34:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.306 210816103199445760 086.42134714368 +48.57123440831 14.8715 14.3053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195001_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195001_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:10.82 +44:51:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.130 197367117487840768 084.79509261774 +44.85611892475 14.7168 13.9121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195004_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 195004_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
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Considering the candidate 195010_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195010_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:52:05.73 +47:55:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.524 210117844596307584 088.02404307541 +47.93237011772 14.7802 14.0439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195011_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195011_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:39:21.48 +46:12:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.165 209547232421774208 084.83992331172 +46.21035976762 14.9478 14.2689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195019_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 195019_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195024_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195024_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:59.69 +44:02:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.840 197111927710804608 084.49902640194 +44.03515731599 14.7286 14.0299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195039_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195039_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:52:09.10 +49:01:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.128 211169080792355968 088.03839458531 +49.01883251602 14.9691 14.2284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195042_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195042_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:43:51.85 +41:39:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.211 192757792945027968 085.96660850387 +41.66113921297 14.5630 13.9268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195045_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 195045_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195051_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195051_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:38:38.98 +42:37:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.119 196003379471527808 084.66319304527 +42.62863555572 14.7922 14.1409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195065_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 195065_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195070_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 195070_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195109_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 195109_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:00:47.24 +44:57:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.139 963015853420168704 090.19662718302 +44.95080844354 14.7279 14.0293 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
Preparing report for the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:57:24.04 +48:22:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:59:44.13 +47:37:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 05:37:57.07 +44:41:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-09_23-20-35_20.00sec_-4.90C_LIGHT_0059 did not pass the final checks
**** FOUND 06:14:58.99 +46:47:46.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 179s
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 ####
06:27:32.18 +42:47:53.2
06:02:41.34 +42:24:32.8
06:01:05.99 +43:45:17.6
05:46:20.81 +41:48:11.7
05:44:06.54 +47:04:03.2
05:41:40.00 +46:46:07.5
05:38:57.32 +43:46:21.5
05:42:39.10 +45:27:02.6
05:39:14.27 +46:12:07.6
06:06:24.49 +44:04:01.4
05:51:24.87 +42:52:21.4
05:56:59.71 +43:04:36.2
05:55:17.32 +42:15:07.6
05:45:00.24 +41:57:14.2
05:48:58.14 +45:32:38.7
06:20:28.95 +43:00:51.7
06:01:34.93 +44:19:46.6
05:40:29.60 +46:12:12.4
05:47:57.02 +44:02:17.3
05:48:55.36 +45:35:44.7
06:04:41.73 +42:52:11.1
05:52:59.28 +46:57:30.7
05:37:19.48 +44:51:38.0
06:27:52.57 +42:46:46.0
06:36:46.04 +42:57:53.1
06:13:19.13 +41:52:42.4
06:24:57.91 +42:35:45.3
05:43:57.15 +41:54:01.0
06:27:15.62 +43:10:36.6
05:54:08.20 +41:46:22.2
05:50:10.20 +43:38:47.5
06:26:12.29 +43:37:29.3
05:50:23.57 +41:49:03.7
05:48:07.42 +45:19:07.0
06:21:01.10 +42:34:37.2
05:48:33.25 +41:48:56.2
05:49:28.93 +44:16:19.5
05:53:06.83 +44:56:00.4
05:52:42.40 +46:52:57.9
06:02:32.09 +48:11:24.8
05:39:19.21 +44:01:56.6
05:45:50.33 +44:23:02.2
05:35:07.78 +46:04:31.5
05:56:33.76 +45:29:09.9
05:49:38.76 +47:49:48.3
05:37:16.41 +44:02:47.4
05:57:12.07 +42:33:34.4
05:42:49.35 +45:57:52.0
05:52:52.05 +42:56:52.8
06:26:29.63 +49:54:10.7
05:39:25.37 +42:39:13.2
05:49:13.41 +41:56:32.8
05:39:33.80 +49:48:36.6
05:58:09.55 +48:37:13.0
05:37:52.47 +43:02:34.2
05:50:47.95 +47:35:35.6
05:53:04.51 +46:18:46.8
05:49:06.60 +47:18:00.3
05:58:27.43 +43:46:24.2
05:35:09.19 +46:30:57.7
05:51:05.26 +47:34:02.9
05:50:56.37 +44:56:18.0
06:10:00.07 +45:32:44.6
05:47:40.55 +44:13:22.4
05:47:48.03 +42:57:38.0
06:09:09.75 +48:13:12.9
06:07:57.19 +48:09:51.1
05:44:33.90 +44:14:46.4
05:53:36.50 +42:34:46.5
06:02:57.90 +43:16:33.9
05:58:11.09 +47:07:48.3
06:00:16.27 +44:41:23.3
05:54:28.12 +43:33:41.7
05:40:39.01 +42:25:36.4
05:37:30.34 +44:27:04.2
05:52:24.51 +43:35:39.4
05:35:52.24 +44:09:06.9
05:51:51.08 +44:14:22.7
05:52:45.30 +44:27:24.2
05:52:55.40 +43:20:10.8
########### 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 ####
06:02:41.34 +42:24:32.8
06:01:05.99 +43:45:17.6
05:46:20.81 +41:48:11.7
05:44:06.54 +47:04:03.2
05:41:40.00 +46:46:07.5
05:38:57.32 +43:46:21.5
05:42:39.10 +45:27:02.6
05:39:14.27 +46:12:07.6
06:06:24.49 +44:04:01.4
05:51:24.87 +42:52:21.4
05:56:59.71 +43:04:36.2
05:55:17.32 +42:15:07.6
05:45:00.24 +41:57:14.2
05:48:58.14 +45:32:38.7
06:20:28.95 +43:00:51.7
06:01:34.93 +44:19:46.6
05:40:29.60 +46:12:12.4
05:47:57.02 +44:02:17.3
05:48:55.36 +45:35:44.7
06:04:41.73 +42:52:11.1
05:52:59.28 +46:57:30.7
05:37:19.48 +44:51:38.0
06:27:52.57 +42:46:46.0
06:36:46.04 +42:57:53.1
06:13:19.13 +41:52:42.4
06:24:57.91 +42:35:45.3
05:43:57.15 +41:54:01.0
06:27:15.62 +43:10:36.6
05:54:08.20 +41:46:22.2
05:50:10.20 +43:38:47.5
06:26:12.29 +43:37:29.3
05:50:23.57 +41:49:03.7
05:48:07.42 +45:19:07.0
06:21:01.10 +42:34:37.2
05:48:33.25 +41:48:56.2
05:49:28.93 +44:16:19.5
05:53:06.83 +44:56:00.4
05:52:42.40 +46:52:57.9
06:02:32.09 +48:11:24.8
05:39:19.21 +44:01:56.6
05:45:50.33 +44:23:02.2
05:35:07.78 +46:04:31.5
05:56:33.76 +45:29:09.9
05:49:38.76 +47:49:48.3
05:37:16.41 +44:02:47.4
05:57:12.07 +42:33:34.4
05:42:49.35 +45:57:52.0
05:52:52.05 +42:56:52.8
06:26:29.63 +49:54:10.7
05:39:25.37 +42:39:13.2
05:49:13.41 +41:56:32.8
05:39:33.80 +49:48:36.6
05:58:09.55 +48:37:13.0
05:37:52.47 +43:02:34.2
05:50:47.95 +47:35:35.6
05:53:04.51 +46:18:46.8
05:49:06.60 +47:18:00.3
05:58:27.43 +43:46:24.2
05:35:09.19 +46:30:57.7
05:51:05.26 +47:34:02.9
05:50:56.37 +44:56:18.0
06:10:00.07 +45:32:44.6
05:47:40.55 +44:13:22.4
05:47:48.03 +42:57:38.0
06:09:09.75 +48:13:12.9
06:07:57.19 +48:09:51.1
05:44:33.90 +44:14:46.4
05:53:36.50 +42:34:46.5
06:02:57.90 +43:16:33.9
05:58:11.09 +47:07:48.3
06:00:16.27 +44:41:23.3
05:54:28.12 +43:33:41.7
05:40:39.01 +42:25:36.4
05:37:30.34 +44:27:04.2
05:52:24.51 +43:35:39.4
05:35:52.24 +44:09:06.9
05:51:51.08 +44:14:22.7
05:52:45.30 +44:27:24.2
05:52:55.40 +43:20:10.8
06:27:32.18 +42:47:53.2
###################################################################################
06:02:41.34 +42:24:32.8 -- not an asteroid (will add it to exclusion list)
06:01:05.99 +43:45:17.6 -- not an asteroid (will add it to exclusion list)
05:46:20.81 +41:48:11.7 -- not an asteroid (will add it to exclusion list)
05:44:06.54 +47:04:03.2 -- not an asteroid (will add it to exclusion list)
05:41:40.00 +46:46:07.5 -- not an asteroid (will add it to exclusion list)
05:38:57.32 +43:46:21.5 -- not an asteroid (will add it to exclusion list)
05:42:39.10 +45:27:02.6 -- not an asteroid (will add it to exclusion list)
05:39:14.27 +46:12:07.6 -- not an asteroid (will add it to exclusion list)
06:06:24.49 +44:04:01.4 -- not an asteroid (will add it to exclusion list)
05:51:24.87 +42:52:21.4 -- not an asteroid (will add it to exclusion list)
05:56:59.71 +43:04:36.2 -- not an asteroid (will add it to exclusion list)
05:55:17.32 +42:15:07.6 -- not an asteroid (will add it to exclusion list)
05:45:00.24 +41:57:14.2 -- not an asteroid (will add it to exclusion list)
05:48:58.14 +45:32:38.7 -- not an asteroid (will add it to exclusion list)
06:20:28.95 +43:00:51.7 -- not an asteroid (will add it to exclusion list)
06:01:34.93 +44:19:46.6 -- not an asteroid (will add it to exclusion list)
05:40:29.60 +46:12:12.4 -- not an asteroid (will add it to exclusion list)
05:47:57.02 +44:02:17.3 -- not an asteroid (will add it to exclusion list)
05:48:55.36 +45:35:44.7 -- not an asteroid (will add it to exclusion list)
06:04:41.73 +42:52:11.1 -- not an asteroid (will add it to exclusion list)
05:52:59.28 +46:57:30.7 -- not an asteroid (will add it to exclusion list)
05:37:19.48 +44:51:38.0 -- not an asteroid (will add it to exclusion list)
06:27:52.57 +42:46:46.0 -- not an asteroid (will add it to exclusion list)
06:36:46.04 +42:57:53.1 -- not an asteroid (will add it to exclusion list)
06:13:19.13 +41:52:42.4 -- not an asteroid (will add it to exclusion list)
06:24:57.91 +42:35:45.3 -- not an asteroid (will add it to exclusion list)
05:43:57.15 +41:54:01.0 -- not an asteroid (will add it to exclusion list)
06:27:15.62 +43:10:36.6 -- not an asteroid (will add it to exclusion list)
05:54:08.20 +41:46:22.2 -- not an asteroid (will add it to exclusion list)
05:50:10.20 +43:38:47.5 -- not an asteroid (will add it to exclusion list)
06:26:12.29 +43:37:29.3 -- not an asteroid (will add it to exclusion list)
05:50:23.57 +41:49:03.7 -- not an asteroid (will add it to exclusion list)
05:48:07.42 +45:19:07.0 -- not an asteroid (will add it to exclusion list)
06:21:01.10 +42:34:37.2 -- not an asteroid (will add it to exclusion list)
05:48:33.25 +41:48:56.2 -- not an asteroid (will add it to exclusion list)
05:49:28.93 +44:16:19.5 -- not an asteroid (will add it to exclusion list)
05:53:06.83 +44:56:00.4 -- not an asteroid (will add it to exclusion list)
05:52:42.40 +46:52:57.9 -- not an asteroid (will add it to exclusion list)
06:02:32.09 +48:11:24.8 -- not an asteroid (will add it to exclusion list)
05:39:19.21 +44:01:56.6 -- not an asteroid (will add it to exclusion list)
05:45:50.33 +44:23:02.2 -- not an asteroid (will add it to exclusion list)
05:35:07.78 +46:04:31.5 -- not an asteroid (will add it to exclusion list)
05:56:33.76 +45:29:09.9 -- not an asteroid (will add it to exclusion list)
05:49:38.76 +47:49:48.3 -- not an asteroid (will add it to exclusion list)
05:37:16.41 +44:02:47.4 -- not an asteroid (will add it to exclusion list)
05:57:12.07 +42:33:34.4 -- not an asteroid (will add it to exclusion list)
05:42:49.35 +45:57:52.0 -- not an asteroid (will add it to exclusion list)
05:52:52.05 +42:56:52.8 -- not an asteroid (will add it to exclusion list)
06:26:29.63 +49:54:10.7 -- not an asteroid (will add it to exclusion list)
05:39:25.37 +42:39:13.2 -- not an asteroid (will add it to exclusion list)
05:49:13.41 +41:56:32.8 -- not an asteroid (will add it to exclusion list)
05:39:33.80 +49:48:36.6 -- not an asteroid (will add it to exclusion list)
05:58:09.55 +48:37:13.0 -- not an asteroid (will add it to exclusion list)
05:37:52.47 +43:02:34.2 -- not an asteroid (will add it to exclusion list)
05:50:47.95 +47:35:35.6 -- not an asteroid (will add it to exclusion list)
05:53:04.51 +46:18:46.8 -- not an asteroid (will add it to exclusion list)
05:49:06.60 +47:18:00.3 -- not an asteroid (will add it to exclusion list)
05:58:27.43 +43:46:24.2 -- not an asteroid (will add it to exclusion list)
05:35:09.19 +46:30:57.7 -- not an asteroid (will add it to exclusion list)
05:51:05.26 +47:34:02.9 -- not an asteroid (will add it to exclusion list)
05:50:56.37 +44:56:18.0 -- not an asteroid (will add it to exclusion list)
06:10:00.07 +45:32:44.6 -- not an asteroid (will add it to exclusion list)
05:47:40.55 +44:13:22.4 -- not an asteroid (will add it to exclusion list)
05:47:48.03 +42:57:38.0 -- not an asteroid (will add it to exclusion list)
06:09:09.75 +48:13:12.9 -- not an asteroid (will add it to exclusion list)
06:07:57.19 +48:09:51.1 -- not an asteroid (will add it to exclusion list)
05:44:33.90 +44:14:46.4 -- not an asteroid (will add it to exclusion list)
05:53:36.50 +42:34:46.5 -- not an asteroid (will add it to exclusion list)
06:02:57.90 +43:16:33.9 -- not an asteroid (will add it to exclusion list)
05:58:11.09 +47:07:48.3 -- not an asteroid (will add it to exclusion list)
06:00:16.27 +44:41:23.3 -- not an asteroid (will add it to exclusion list)
05:54:28.12 +43:33:41.7 -- not an asteroid (will add it to exclusion list)
05:40:39.01 +42:25:36.4 -- not an asteroid (will add it to exclusion list)
05:37:30.34 +44:27:04.2 -- not an asteroid (will add it to exclusion list)
05:52:24.51 +43:35:39.4 -- not an asteroid (will add it to exclusion list)
05:35:52.24 +44:09:06.9 -- not an asteroid (will add it to exclusion list)
05:51:51.08 +44:14:22.7 -- not an asteroid (will add it to exclusion list)
05:52:45.30 +44:27:24.2 -- not an asteroid (will add it to exclusion list)
05:52:55.40 +43:20:10.8 -- not an asteroid (will add it to exclusion list)
06:27:32.18 +42:47:53.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:35:07.78 +46:04:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:09.19 +46:30:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:52.24 +44:09:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.41 +44:02:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.48 +44:51:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:30.34 +44:27:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.47 +43:02:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:57.32 +43:46:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:14.27 +46:12:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.21 +44:01:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:25.37 +42:39:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:33.80 +49:48:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:29.60 +46:12:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:39.01 +42:25:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:40.00 +46:46:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:39.10 +45:27:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:49.35 +45:57:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:57.15 +41:54:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:06.54 +47:04:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:33.90 +44:14:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:00.24 +41:57:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.33 +44:23:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:20.81 +41:48:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:40.55 +44:13:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:48.03 +42:57:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:57.02 +44:02:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:07.42 +45:19:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:33.25 +41:48:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:55.36 +45:35:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:58.14 +45:32:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.60 +47:18:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:13.41 +41:56:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.93 +44:16:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.76 +47:49:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.20 +43:38:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.57 +41:49:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:47.95 +47:35:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:56.37 +44:56:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:05.26 +47:34:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:24.87 +42:52:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:51.08 +44:14:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:24.51 +43:35:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:42.40 +46:52:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:45.30 +44:27:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:52.05 +42:56:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:55.40 +43:20:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:59.28 +46:57:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.51 +46:18:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.83 +44:56:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:36.50 +42:34:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:08.20 +41:46:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:28.12 +43:33:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:17.32 +42:15:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.76 +45:29:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:59.71 +43:04:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:12.07 +42:33:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.55 +48:37:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:11.09 +47:07:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.43 +43:46:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:16.27 +44:41:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:05.99 +43:45:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:34.93 +44:19:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.09 +48:11:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:41.34 +42:24:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:57.90 +43:16:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:41.73 +42:52:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:24.49 +44:04:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:57.19 +48:09:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:09.75 +48:13:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:00.07 +45:32:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:19.13 +41:52:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:28.95 +43:00:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:01.10 +42:34:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:57.91 +42:35:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:12.29 +43:37:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.63 +49:54:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:15.62 +43:10:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:32.18 +42:47:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:52.57 +42:46:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:46.04 +42:57:53.1 -- 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)
05:35:07.78 +46:04:31.5 -- not a known variable star
05:35:09.19 +46:30:57.7 -- not a known variable star
05:35:52.24 +44:09:06.9 -- not a known variable star
05:37:16.41 +44:02:47.4 -- not a known variable star
05:37:19.48 +44:51:38.0 -- not a known variable star
05:37:30.34 +44:27:04.2 -- a known variable star
05:37:52.47 +43:02:34.2 -- not a known variable star
05:38:57.32 +43:46:21.5 -- not a known variable star
05:39:14.27 +46:12:07.6 -- not a known variable star
05:39:19.21 +44:01:56.6 -- not a known variable star
05:39:25.37 +42:39:13.2 -- not a known variable star
05:39:33.80 +49:48:36.6 -- not a known variable star
05:40:29.60 +46:12:12.4 -- not a known variable star
05:40:39.01 +42:25:36.4 -- a known variable star
05:41:40.00 +46:46:07.5 -- not a known variable star
05:42:39.10 +45:27:02.6 -- not a known variable star
05:42:49.35 +45:57:52.0 -- not a known variable star
05:43:57.15 +41:54:01.0 -- a known variable star
05:44:06.54 +47:04:03.2 -- not a known variable star
05:44:33.90 +44:14:46.4 -- not a known variable star
05:45:00.24 +41:57:14.2 -- not a known variable star
05:45:50.33 +44:23:02.2 -- not a known variable star
05:46:20.81 +41:48:11.7 -- not a known variable star
05:47:40.55 +44:13:22.4 -- not a known variable star
05:47:48.03 +42:57:38.0 -- not a known variable star
05:47:57.02 +44:02:17.3 -- a known variable star
05:48:07.42 +45:19:07.0 -- not a known variable star
05:48:33.25 +41:48:56.2 -- not a known variable star
05:48:55.36 +45:35:44.7 -- not a known variable star
05:48:58.14 +45:32:38.7 -- not a known variable star
05:49:06.60 +47:18:00.3 -- not a known variable star
05:49:13.41 +41:56:32.8 -- not a known variable star
05:49:28.93 +44:16:19.5 -- not a known variable star
05:49:38.76 +47:49:48.3 -- not a known variable star
05:50:10.20 +43:38:47.5 -- not a known variable star
05:50:23.57 +41:49:03.7 -- not a known variable star
05:50:47.95 +47:35:35.6 -- a known variable star
05:50:56.37 +44:56:18.0 -- not a known variable star
05:51:05.26 +47:34:02.9 -- not a known variable star
05:51:24.87 +42:52:21.4 -- not a known variable star
05:51:51.08 +44:14:22.7 -- not a known variable star
05:52:24.51 +43:35:39.4 -- not a known variable star
05:52:42.40 +46:52:57.9 -- not a known variable star
05:52:45.30 +44:27:24.2 -- not a known variable star
05:52:52.05 +42:56:52.8 -- a known variable star
05:52:55.40 +43:20:10.8 -- not a known variable star
05:52:59.28 +46:57:30.7 -- not a known variable star
05:53:04.51 +46:18:46.8 -- not a known variable star
05:53:06.83 +44:56:00.4 -- not a known variable star
05:53:36.50 +42:34:46.5 -- a known variable star
05:54:08.20 +41:46:22.2 -- a known variable star
05:54:28.12 +43:33:41.7 -- not a known variable star
05:55:17.32 +42:15:07.6 -- not a known variable star
05:56:33.76 +45:29:09.9 -- not a known variable star
05:56:59.71 +43:04:36.2 -- not a known variable star
05:57:12.07 +42:33:34.4 -- not a known variable star
05:58:09.55 +48:37:13.0 -- not a known variable star
05:58:11.09 +47:07:48.3 -- not a known variable star
05:58:27.43 +43:46:24.2 -- not a known variable star
06:00:16.27 +44:41:23.3 -- not a known variable star
06:01:05.99 +43:45:17.6 -- not a known variable star
06:01:34.93 +44:19:46.6 -- not a known variable star
06:02:32.09 +48:11:24.8 -- not a known variable star
06:02:41.34 +42:24:32.8 -- not a known variable star
06:02:57.90 +43:16:33.9 -- not a known variable star
06:04:41.73 +42:52:11.1 -- not a known variable star
06:06:24.49 +44:04:01.4 -- not a known variable star
06:07:57.19 +48:09:51.1 -- not a known variable star
06:09:09.75 +48:13:12.9 -- not a known variable star
06:10:00.07 +45:32:44.6 -- not a known variable star
06:13:19.13 +41:52:42.4 -- not a known variable star
06:20:28.95 +43:00:51.7 -- not a known variable star
06:21:01.10 +42:34:37.2 -- not a known variable star
06:24:57.91 +42:35:45.3 -- not a known variable star
06:26:12.29 +43:37:29.3 -- a known variable star
06:26:29.63 +49:54:10.7 -- not a known variable star
06:27:15.62 +43:10:36.6 -- not a known variable star
06:27:32.18 +42:47:53.2 -- not a known variable star
06:27:52.57 +42:46:46.0 -- not a known variable star
06:36:46.04 +42:57:53.1 -- not a known variable star
Found 71 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
80 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 80 (excluding asteroids and hot pixels, 71 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)2461140.68048054 -observatory V36
23:38:11.74 -04:54:58.7 Mercury (0.2mag)
02:40:28.34 +15:33:20.2 Venus (-3.9mag)
00:01:17.21 -00:57:30.4 Mars (1.2mag)
07:10:10.15 +22:50:11.1 Jupiter (-2.1mag)
00:26:34.16 +00:32:37.7 Saturn (0.9mag)
03:46:30.13 +19:43:37.7 Uranus (5.8mag)
00:10:04.13 -00:20:14.8 Neptune (7.8mag)
20:33:28.11 -22:52:27.0 Pluto (14.5mag)
19:30:11.85 -26:00:07.0 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Apr 9 23:36 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461140.68048054:
07:10:03.19 +22:50:23.5 Io (5.7mag)
07:10:18.00 +22:49:52.2 Europa (5.9mag)
07:10:08.74 +22:50:06.3 Ganymede (5.3mag)
07:09:48.59 +22:51:01.2 Callisto (6.6mag)
07:13:44.71 +22:40:37.7 Himalia (15.3mag)
07:10:06.21 +22:50:19.8 Thebe (16.2mag)
07:13:48.19 +23:10:09.6 Elara (17.3mag)
07:08:39.26 +23:33:14.1 Pasiphae (17.4mag)
07:18:37.29 +22:47:35.7 Carme (18.5mag)
00:26:44.06 +00:32:28.5 Titan (8.8mag)
00:26:33.00 +00:32:53.8 Rhea (10.1mag)
00:26:25.70 +00:33:40.6 Iapetus (11.5mag)
00:26:47.69 +00:32:26.4 Hyperion (14.8mag)
00:28:15.53 +00:42:02.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 23:37 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.68048054:
15:10:02.28 -11:49:00.3 JWST
19:17:47.16 +13:36:47.2 Chandra
07:58:46.33 -37:33:35.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 23:36 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.68048054 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:19.68 -28:26:54.8 13.9mag P/2010 H2 (Vales)
05:02:41.16 -69:56:41.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:16.13 +31:23:58.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:51.30 +09:51:09.2 17.6mag C/2021 G2 (ATLAS)
23:08:35.17 +29:00:25.9 17.0mag C/2022 E2 (ATLAS)
04:22:30.88 +25:52:39.8 15.9mag C/2022 N2 (PANSTARRS)
09:02:21.29 +31:57:56.9 16.2mag C/2022 QE78 (ATLAS)
08:30:19.15 -00:46:59.6 17.3mag C/2022 R6 (PANSTARRS)
18:54:57.30 +18:02:19.3 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:26.94 -11:36:20.1 17.5mag P/2023 B1 (PANSTARRS)
09:10:32.96 -12:49:56.0 17.6mag C/2023 F3 (ATLAS)
21:48:04.32 +62:34:41.8 17.5mag C/2023 H5 (Lemmon)
19:23:47.78 -03:38:59.8 14.2mag C/2023 R1 (PANSTARRS)
21:40:34.20 +85:07:20.8 17.8mag C/2023 X2 (Lemmon)
06:15:34.81 +63:32:53.6 17.1mag C/2024 A1 (ATLAS)
05:00:25.07 +16:12:53.0 10.7mag C/2024 E1 (Wierzchos)
16:22:51.68 +05:26:03.0 17.4mag C/2024 G6 (ATLAS)
20:19:00.38 +13:43:04.4 14.7mag C/2024 J3 (ATLAS)
03:21:12.51 -23:17:10.6 16.4mag C/2024 T5 (ATLAS)
05:11:52.39 +46:46:16.7 17.7mag C/2025 J1 (Borisov)
14:02:58.87 +41:07:19.9 14.9mag C/2025 L1 (ATLAS)
03:16:16.50 -25:19:36.7 17.8mag C/2025 Q3 (ATLAS)
23:06:46.61 +19:42:36.6 9.4mag C/2025 R3 (PANSTARRS)
12:56:39.15 +02:39:01.5 17.5mag C/2025 Y1 (ATLAS)
02:30:05.21 +03:30:05.1 10.9mag C/2026 A1 (MAPS)
23:42:45.37 +36:05:34.6 14.4mag C/2026 B2 (Sun-Gao)
18:31:35.32 -10:01:23.8 12.2mag 10P/Tempel
15:08:00.37 +03:46:30.9 13.5mag 24P/Schaumasse
11:04:28.60 -01:43:16.7 15.7mag 29P/Schwassmann-Wachmann
17:58:49.47 -09:49:56.5 17.8mag 40P/Vaisala
10:38:06.55 -04:35:07.5 16.8mag 43P/Wolf-Harrington
01:39:41.01 +16:29:21.1 17.2mag 47P/Ashbrook-Jackson
07:00:14.08 +38:15:00.1 17.0mag 63P/Wild
23:21:33.32 -12:09:31.2 15.7mag 65P/Gunn
03:47:54.43 +19:12:21.5 15.9mag 76P/West-Kohoutek-Ikemura
00:52:46.13 +07:04:45.6 14.4mag 78P/Gehrels
22:45:07.88 -11:06:27.2 14.6mag 88P/Howell
01:54:06.14 +19:03:48.7 15.1mag 93P/Lovas
04:44:01.82 +31:57:54.2 16.3mag 123P/West-Hartley
08:21:51.84 +41:02:55.1 16.2mag 124P/Mrkos
02:24:16.32 +13:42:52.1 16.4mag 128P/Shoemaker-Holt
02:36:09.10 +13:46:08.4 17.5mag 131P/Mueller
00:55:58.70 +11:08:30.8 10.9mag 141P/Machholz
01:05:37.06 +02:41:14.3 11.0mag 141P-A/Machholz
23:53:54.41 -01:09:10.2 13.5mag 141P-D/Machholz
01:35:19.80 +04:24:29.1 17.9mag 141P-I/Machholz
00:46:11.17 -04:26:29.3 15.2mag 162P/SidingSpring
10:29:51.17 +31:15:06.6 17.9mag 164P/Christensen
06:25:45.13 +24:25:18.1 17.9mag 198P/ODAS
15:01:45.55 -00:42:31.6 17.5mag 210P/Christensen
21:21:30.14 -12:51:21.6 17.5mag 218P/LINEAR
17:14:36.46 -14:37:15.6 16.2mag 235P/LINEAR
05:22:01.50 +34:13:30.6 16.7mag 240P/NEAT
07:35:48.25 -05:48:59.4 17.7mag 242P/Spahr
15:44:44.56 +06:35:40.4 17.5mag 391P/Kowalski
07:32:07.17 +21:20:24.6 17.6mag 450P/LONEOS
05:27:29.54 +45:22:28.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 23:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 9 23:36 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 23:36 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:18:48.927 -23:32:12.08 AT 2026ike 2026-02-12.51 20.2
08:47:41.490 -21:46:40.10 AT 2026ikd 2026-03-28.41 19.49
08:34:30.248 -07:09:24.85 AT 2026ikc 2026-03-29.44 19.28
13:21:25.078 +79:09:18.53 AT 2026ikb 2026-03-25.43 20.7322
09:05:18.124 -19:48:21.41 AT 2026ika 2026-03-09.36 20.58
08:38:25.468 +06:11:03.79 AT 2026ijz 2026-03-09.32 21.99
08:00:34.010 +04:48:18.04 AT 2026ijy 2026-03-09.31 21.07
09:02:07.082 +07:27:03.87 AT 2026ijx 2026-02-17.43 21.29
10:37:20.784 +30:59:50.95 AT 2026ijw 2026-03-10.33 20.2
16:00:37.915 +06:38:30.61 AT 2026ijv 2026-03-28.57 20.5
13:51:30.137 +25:53:04.17 AT 2026iju 2026-03-28.41 20.07
12:52:01.341 -19:06:48.80 AT 2026ijt 2026-01-28.59 20.22
11:38:25.995 -11:34:40.48 AT 2026ijs 2026-01-16.56 21.1
07:12:41.661 +56:25:20.59 AT 2026ijr 2026-01-19.40 20.76
09:34:48.813 +06:57:40.76 AT 2026ijq 2026-01-26.43 21.57
10:49:59.384 +25:17:19.22 AT 2026ijp 2026-04-04.17 19.836
08:20:22.449 +03:44:22.06 AT 2026ijo 2026-04-02.18 19.8276
06:41:34.987 -19:08:36.17 AT 2026ijn 2026-02-05.26 20.38
12:35:13.975 +41:45:24.96 AT 2026ijm 2026-04-02.31 19.9925
13:25:11.624 +08:21:44.99 AT 2026ijl 2026-03-27.40 20.8103
-rw-r--r-- 1 apache apache 30K Apr 9 23:36 tns_transients_list.txt
