This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF
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,2461144.6388,13.75,0.05,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
target 20260414.1388 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
Gaia DR3 969680749309131648,2461144.6388,13.74,0.05,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
Gaia DR3 969680749309131648 20260414.1388 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 J088.3489+43.4595,2461144.6388,13.74,0.05,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 J088.3489+43.4595 20260414.1388 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.62,0.05,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
target 20260414.1388 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461144.6388,13.60,0.05,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
Gaia DR3 197994904265884544 20260414.1388 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
ASASSN-V J055127.94+451129.9,2461144.6388,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J055127.94+451129.9 20260414.1388 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3686+43.2939,2461144.6388,13.10,0.05,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 J084.3686+43.2939 20260414.1388 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461144.6388,13.17,0.05,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 20260414.1388 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.1267+46.2073,2461144.6388,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.1267+46.2073 20260414.1388 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194772338765794816,2461144.6388,13.05,0.05,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
Gaia DR3 194772338765794816 20260414.1388 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 J093.2860+45.0831,2461144.6388,12.88,0.05,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
ATO J093.2860+45.0831 20260414.1388 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210566788938313216,2461144.6388,13.04,0.05,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
Gaia DR3 210566788938313216 20260414.1388 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,2461144.6388,12.88,0.05,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
target 20260414.1388 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060214.12+474700.6,2461144.6388,12.88,0.05,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
ASASSN-V J060214.12+474700.6 20260414.1388 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 961843288690903296,2461144.6388,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 961843288690903296 20260414.1388 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2531+46.4397,2461144.6388,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2531+46.4397 20260414.1388 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.88,0.05,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
target 20260414.1388 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.0519+42.7763,2461144.6388,12.78,0.05,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
ATO J087.0519+42.7763 20260414.1388 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1430+48.5601,2461144.6388,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.1430+48.5601 20260414.1388 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192293833399060608,2461144.6388,12.55,0.05,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 20260414.1388 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.05,0.05,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 20260414.1388 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J097.9916+45.0089,2461144.6388,12.09,0.05,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
ATO J097.9916+45.0089 20260414.1388 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062013.27+433839.0,2461144.6388,11.87,0.05,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
ASASSN-V J062013.27+433839.0 20260414.1388 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 14.1388 2461144.6388 11.40 05:58:32.71 +44:49:13.1
167.48691 10.19581 galactic Aur Second-epoch detections are separated by 0.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 196654530872953984 | 05:58:30.58 +44:49:17.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.454+/-0.028 (G)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 196654530872953984,2461144.6388,11.40,0.05,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
Large-amplitude variable Gaia DR2 196654530872953984 20260414.1388 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193418049677781632,2461144.6388,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193418049677781632 20260414.1388 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 959056340249435648,2461144.6388,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 959056340249435648 20260414.1388 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3774+41.9686,2461144.6388,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3774+41.9686 20260414.1388 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210193191206491904,2461144.6388,12.89,0.05,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
Gaia DR3 210193191206491904 20260414.1388 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
ATO J089.9948+43.8619,2461144.6388,12.89,0.05,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 J089.9948+43.8619 20260414.1388 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
Gaia DR3 968835396666764416,2461144.6388,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 968835396666764416 20260414.1388 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461144.6388,12.93,0.05,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 20260414.1388 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.89,0.05,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
target 20260414.1388 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,2461144.6388,12.95,0.05,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 20260414.1388 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.96,0.05,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 20260414.1388 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461144.6388,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197388553666998656 20260414.1388 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2822+43.1225,2461144.6388,13.04,0.05,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 J089.2822+43.1225 20260414.1388 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,2461144.6388,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195999702979561088,2461144.6388,12.96,0.05,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
Gaia DR3 195999702979561088 20260414.1388 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 J085.7069+47.1882,2461144.6388,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.7069+47.1882 20260414.1388 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461144.6388,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.1629+50.0440 20260414.1388 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.0334+45.0349,2461144.6388,12.92,0.05,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 J092.0334+45.0349 20260414.1388 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.7593+47.5882,2461144.6388,13.10,0.05,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 J084.7593+47.5882 20260414.1388 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260414.1388 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197288807346758784,2461144.6388,13.21,0.05,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 197288807346758784 20260414.1388 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.13,0.05,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
target 20260414.1388 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 196588835052997760,2461144.6388,13.20,0.05,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 196588835052997760 20260414.1388 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461144.6388,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196552271996570368 20260414.1388 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.2884+47.3636,2461144.6388,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.2884+47.3636 20260414.1388 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.28,0.05,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 20260414.1388 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6873+48.2843,2461144.6388,13.30,0.05,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 J092.6873+48.2843 20260414.1388 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 J091.0747+46.9169,2461144.6388,13.27,0.05,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 J091.0747+46.9169 20260414.1388 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2390+42.2966,2461144.6388,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.2390+42.2966 20260414.1388 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192299880712537088,2461144.6388,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192299880712537088 20260414.1388 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.53,0.05,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 20260414.1388 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.5245+41.9504,2461144.6388,13.66,0.05,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
ATO J085.5245+41.9504 20260414.1388 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.71,0.05,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
target 20260414.1388 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461144.6388,13.71,0.05,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
target 20260414.1388 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
## 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: 2461144.63912278 14.04.2026 03:20:10.208 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16248
Objects passed selection criteria: 16212
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 13829.8
Average stars matched: 13475.8 (97.4403 %)
Memory usage VmPeak: 122840 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:28:56 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: 2461144.63912278 14.04.2026 03:20:10.208 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 231
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): 122302
Objects passed selection criteria: 122006
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: 108081
Average stars matched: 104481 (96.6687 %)
Memory usage VmPeak: 1960408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 22:31:42 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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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: 2461144.63846649
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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 06:00:00.393 +46:00:21.83
Angular distance between the image centers 0.0366 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 06:00:01.391 +45:59:43.23
Angular distance between the image centers 0.0419 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 06:00:00.393 +46:00:21.83
Second-epoch second image center 06:00:01.391 +45:59:43.23
Angular distance between the image centers 0.01111 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.73Vs2j5GNM
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.iNLQmq8mIe
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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits &> /tmp/tmp.jf2lqrN5QG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits &> /tmp/tmp.160bDnIqZO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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 3 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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
2.7 pix fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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
14.8 mag. fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
14.7 mag. fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (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.73Vs2j5GNM (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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.iNLQmq8mIe (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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.jf2lqrN5QG (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=927, passed=15339
Got 15339 stars (including 14401 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat
util/solve_plate_with_UCAC5 got 15339 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 15034 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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 15034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 15034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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.160bDnIqZO (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=930, passed=15025
Got 15025 stars (including 14086 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat
util/solve_plate_with_UCAC5 got 15025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 14759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 14757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 14757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 31154_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 31154_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:14:59.01 +46:47:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31159_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 31159_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 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 31272_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 31272_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:45:42.91 +43:37:26.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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 06:00:00.393 +46:00:21.83
Angular distance between the image centers 0.0366 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 06:00:01.391 +45:59:43.23
Angular distance between the image centers 0.0419 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 06:00:00.393 +46:00:21.83
Second-epoch second image center 06:00:01.391 +45:59:43.23
Angular distance between the image centers 0.01111 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.c2VnCeoSpf
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.lky2q0J37E
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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits &> /tmp/tmp.5PB2BfhAGa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits &> /tmp/tmp.2Br3Izvbv1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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 193 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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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
13.9 mag. fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
13.8 mag. fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.c2VnCeoSpf (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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.lky2q0J37E (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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.5PB2BfhAGa (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=9661, passed=110545
Got 110545 stars (including 100769 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat
util/solve_plate_with_UCAC5 got 110545 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 108345 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 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 108346 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 108347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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.2Br3Izvbv1 (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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=9114, passed=108267
Got 108267 stars (including 99042 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat
util/solve_plate_with_UCAC5 got 108267 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 106384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 106384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 106384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
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_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/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_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-19-13_20.00sec_-5.00C_LIGHT_0687.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.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_2026-04-13_CI_Aur-02-Q2b1x1_222057_TTUQ2b1x1_3146_YFgwmYlF/wcs_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out192150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192195.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__out192205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193988.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out192102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192228.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__out192233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194580.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 95s
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: 41s
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Considering the candidate 192102_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192102_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192104_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192104_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192107_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192107_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192114_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192114_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192120_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192120_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192122_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192122_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192131_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192131_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192150_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192150_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:12.79 +44:18:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.301 197083787085249024 085.55409525404 +44.30225092962 14.2648 13.6264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192158_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192158_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:17.10 +47:02:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192170_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192170_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:29.79 +44:43:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.561 197245312213914112 085.62462940332 +44.71832749944 13.8957 13.2499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192171_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192171_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192173_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192173_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192174_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192174_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:14:39.76 +44:54:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.421 962443145300331008 093.66577241718 +44.91289522274 14.2723 13.6786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192178_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192178_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:24.91 +45:43:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.339 209501087293588224 084.35462223877 +45.72979338931 14.0253 13.1241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192182_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192182_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192193_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192193_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192195_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192195_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:30.25 +43:50:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.379 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192201_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192201_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:39:27.54 +45:00:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.448 197372030930368768 084.86570879013 +45.00461244286 14.2352 13.4459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192202_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192202_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:00.29 +42:27:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.332 194494368482144896 084.25126338216 +42.45554787083 13.8924 13.0809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192205_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192205_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:59:43.75 +47:14:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.443 197875298016711168 089.93213850671 +47.23512873704 13.9294 13.3794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192214_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192214_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:38:12.57 +45:11:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192215_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192215_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:37:04.29 +43:10:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.930 964125535529068544 099.26717300104 +43.17835388769 13.7359 12.9234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192216_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192216_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:45:09.22 +48:42:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192219_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192219_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192222_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192222_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192223_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192223_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:27:52.61 +42:46:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.188 958990197753107968 096.96879924143 +42.77921991317 13.8157 13.7262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192228_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192228_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192229_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192229_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192233_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192233_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192235_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:44:36.92 +46:43:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192238_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192238_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192243_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192243_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:26:53.41 +43:56:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192248_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192248_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192252_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192252_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192254_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192254_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:36:57.78 +44:14:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192261_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192261_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:16:36.26 +44:32:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.794 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192262_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192262_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:24.27 +42:05:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192267_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192267_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:00:23.87 +45:45:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192268_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192268_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:52:42.91 +41:55:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.088 192307714733015552 088.17919775815 +41.91970387825 13.2046 12.6297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192271_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192271_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:29.16 +42:21:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.975 195981556740515584 084.37181996051 +42.35539595793 13.2444 12.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192272_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192272_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:44:58.15 +47:20:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192273_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192273_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192274_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192274_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:31:06.94 +48:10:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192275_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192275_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:11:13.09 +47:02:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192276_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192276_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:01.67 +46:28:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192280_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192280_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:17.31 +42:28:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192281_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192281_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:53:59.22 +45:07:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.890 196896423430974720 088.49708655417 +45.12523587564 12.8133 12.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192282_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192282_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:01:39.42 +45:44:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.256 963145561432116224 090.41445434671 +45.73787381455 13.0287 12.5054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192283_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192283_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:00:34.54 +45:32:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.802 963062342146066432 090.14422902412 +45.53343101528 12.7393 12.0346 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 192285_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192285_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192286_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192286_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:41:47.78 +41:45:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192287_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192287_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:21:39.48 +42:45:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.601 961571060781170816 095.41409926265 +42.75244472102 12.6004 12.1625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192288_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192288_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:23.56 +49:53:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192289_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192289_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:23.75 +44:31:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192291_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192291_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:55.25 +42:54:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 0.928 196195961507760768 084.48025002876 +42.90529955301 12.0708 11.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192295_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 192295_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 192296_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192296_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:45.90 +43:34:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192298_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192298_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:09.00 +46:13:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192300_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192300_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:27.56 +42:19:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192431_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192431_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:22.93 +46:49:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192552_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192552_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:45:42.92 +43:37:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192610_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192610_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:11:34.49 +48:44:35.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192711_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192711_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:51:47.60 +48:44:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192748_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192748_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:46:26.48 +47:55:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192808_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192808_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:19:04.18 +47:21:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192833_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192833_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:06:21.30 +48:46:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192932_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192932_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:07.53 +50:04:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192956_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192956_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:39:07.59 +44:53:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192978_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 192978_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:03.02 +42:12:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193015_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193015_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:13:46.65 +44:43:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193020_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193020_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:34:37.48 +45:55:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193042_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193042_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:05:50.19 +44:39:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193056_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193056_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:48:45.95 +46:35:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193081_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193081_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:48:04.09 +43:19:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193094_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193094_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193120_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193120_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:03:13.60 +42:56:26.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193121_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193121_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:42.96 +48:20:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193161_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193161_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:47:16.18 +46:04:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193176_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193176_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:53:12.05 +45:24:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193187_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193187_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:52.82 +47:06:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193189_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193189_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:32.56 +43:42:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193204_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193204_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:25.88 +48:47:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193210_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193210_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193218_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193218_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:47:45.26 +50:03:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193220_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193220_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:46.12 +45:53:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193262_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193262_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 193266_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193266_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:14.17 +50:00:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193277_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193277_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:11:01.02 +47:29:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193280_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193280_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:46.28 +43:03:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193324_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193324_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:01:04.62 +50:00:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193355_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193355_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:44:48.23 +48:58:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193358_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193358_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:17:34.69 +46:23:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193366_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193366_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:44.76 +44:40:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.597 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193382_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193382_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:17.33 +46:01:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193400_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193400_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:34:02.67 +46:44:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193404_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193404_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:46.40 +46:04:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193410_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193410_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:39:32.63 +41:57:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193428_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193428_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:00:14.05 +47:43:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193433_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193433_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:08:02.26 +46:40:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.629 963435214026488704 092.00979468381 +46.68289863325 13.5967 13.1319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193440_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193440_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:06.55 +44:51:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193474_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193474_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:14.56 +43:32:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193497_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193497_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:52:03.61 +49:32:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193506_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193506_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193524_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193524_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:24.31 +42:59:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193555_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193555_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193563_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193563_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193566_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193566_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:35:35.23 +44:15:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193577_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193577_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:48:23.27 +49:46:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.178 211485637061247744 087.09740055049 +49.78256265660 13.8223 13.2232 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 193580_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193580_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:28.20 +42:14:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193582_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193582_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193584_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193584_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:44:39.72 +43:57:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193585_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193585_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:22.09 +42:59:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193591_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193591_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:31.29 +47:51:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.477 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193623_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193623_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:53:31.08 +44:15:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.399 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 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 193635_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193635_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:17:15.75 +41:56:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.862 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193647_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193647_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:30.03 +44:44:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193653_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193653_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:50.67 +48:07:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.475 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193670_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193670_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193680_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193680_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:46:39.74 +43:21:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.658 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193692_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193692_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193693_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193693_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193696_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193696_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193729_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193729_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:18.68 +47:12:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.967 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193732_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193732_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193737_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193737_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:50.53 +49:49:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193742_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193742_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:25:45.21 +45:22:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193746_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193746_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:24.81 +49:14:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.490 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193764_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193764_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:40:59.45 +46:21:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193776_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193776_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:27.86 +47:51:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.391 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193777_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193777_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193786_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193786_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193789_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193789_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193799_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193799_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193801_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193801_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:25.51 +42:20:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.158 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193811_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193811_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193830_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193830_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:39:18.48 +44:01:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193834_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193834_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:06.23 +45:12:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193836_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193836_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193840_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193840_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:51:18.84 +43:17:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 0.784 193427528667708288 087.82879815788 +43.29576806055 13.9092 13.2559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193857_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193857_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193858_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193858_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:03:43.61 +50:12:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193860_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193860_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:50:06.47 +46:08:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193867_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193867_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:55:50.62 +42:45:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193869_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193869_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193874_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193874_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:38.65 +47:49:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.361 210278579453256064 087.41194921401 +47.83006271100 14.1312 13.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193888_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193888_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193938_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193938_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193947_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193947_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:03:21.17 +42:41:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.716 960875035561541376 090.83923379420 +42.69689639166 13.9565 13.4004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193949_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 193949_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 193954_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193954_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:56.71 +47:43:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.993 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193971_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193971_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:52:21.10 +42:50:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193974_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193974_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:35:41.27 +44:16:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193988_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193988_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:56:28.37 +47:43:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.034 210132688003360128 089.11859936957 +47.72833351240 14.2142 13.3827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193990_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 193990_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:48:44.71 +49:34:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.849 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194019_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194019_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194028_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194028_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194050_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194050_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:39:33.83 +49:48:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.548 214254688376903680 084.89157910286 +49.80984354835 14.2849 13.7457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194066_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194066_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:55.46 +45:00:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194073_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194073_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194083_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194083_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:42:16.18 +43:16:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194086_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194086_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:53.18 +46:05:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194105_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194105_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:12:19.98 +50:12:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194107_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194107_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:53:58.70 +46:09:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194118_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194118_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194125_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194125_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194144_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194144_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194156_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194156_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194165_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194165_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:41:07.32 +47:58:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194179_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194179_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:07.19 +47:47:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.407 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194184_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194184_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194243_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194243_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:17:15.23 +42:06:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194249_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194249_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194313_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194313_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:38:34.87 +44:30:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.087 197324992449032448 084.64566956412 +44.51452500122 14.4798 13.9246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194336_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194336_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:36:17.15 +47:13:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.039 210617710070467968 084.07227560775 +47.21810814441 14.3191 13.6514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194377_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194377_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:10:00.29 +45:32:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.526 963235820168851712 092.50109436752 +45.54496087176 14.4482 13.9808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194418_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194418_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194451_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194451_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194462_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194462_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 194497_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194497_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
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Considering the candidate 194545_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194545_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:49:39.70 +41:46:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.756 192338702920071936 087.41563650102 +41.78259080838 14.4778 13.7414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194563_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194563_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:43:22.52 +46:37:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.663 209643611488033536 085.84447687391 +46.61743977348 14.6865 13.7367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194577_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194577_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194580_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
Preparing report for the candidate 194580_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194601_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 194601_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:52:47.13 +44:31:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.156 196585467798665600 088.19677367178 +44.52709383905 14.7170 14.1455 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:59:44.11 +47:37:00.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:57:24.03 +48:22:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 05:37:57.14 +44:41:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-13_22-20-10_20.00sec_-4.90C_LIGHT_0688 did not pass the final checks
**** FOUND 06:14:58.98 +46:47:46.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 140s
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 ####
05:55:50.61 +46:34:58.5
06:06:53.96 +48:50:11.6
05:53:23.62 +43:27:34.5
05:36:44.15 +43:04:49.3
05:56:05.28 +44:35:31.2
05:56:52.39 +43:51:21.8
05:53:04.86 +46:58:02.5
05:51:27.67 +45:11:26.4
05:56:14.85 +48:35:48.1
05:37:29.65 +43:17:37.0
05:52:59.33 +46:57:31.1
05:40:29.48 +46:12:11.1
05:35:49.54 +43:04:58.2
06:13:09.47 +45:05:09.4
05:35:09.96 +46:58:05.6
06:35:49.95 +48:37:47.4
06:02:14.37 +47:47:00.4
06:16:04.85 +43:18:56.4
05:56:59.32 +46:26:55.8
06:08:44.09 +48:20:44.4
05:48:13.23 +42:46:42.2
06:00:35.20 +48:33:25.3
05:54:07.84 +41:46:23.6
06:25:08.20 +42:30:49.3
06:31:57.28 +45:00:41.7
06:20:12.71 +43:38:54.5
05:58:32.71 +44:49:13.1
06:12:10.23 +50:14:53.5
06:26:19.92 +41:59:08.5
05:53:17.73 +43:17:15.4
06:25:57.22 +43:06:04.9
06:13:29.56 +41:58:05.4
05:54:13.39 +47:53:37.4
05:59:58.97 +43:51:29.8
06:13:33.54 +48:03:16.7
06:02:32.06 +48:11:24.9
05:57:45.30 +45:54:52.2
06:26:29.60 +49:54:11.0
05:57:11.25 +42:50:25.8
05:37:19.39 +44:51:38.5
05:57:07.90 +43:07:28.5
06:00:04.32 +45:58:32.6
05:37:44.70 +42:36:38.6
05:42:53.55 +47:11:05.6
05:36:40.84 +50:02:54.9
06:08:04.94 +45:02:04.4
05:39:18.97 +44:01:55.4
05:38:59.94 +47:35:32.1
05:41:02.57 +46:20:39.0
05:46:32.87 +45:16:05.6
05:37:52.40 +43:02:35.5
05:52:57.86 +44:33:10.5
05:50:28.69 +44:11:34.4
06:01:02.32 +47:22:14.5
05:49:08.62 +44:09:11.8
06:10:45.00 +48:16:56.3
06:04:15.55 +46:54:36.7
05:52:55.17 +42:18:28.1
05:54:16.08 +41:58:03.4
05:44:02.82 +45:51:12.0
05:42:06.12 +41:56:49.5
05:50:56.43 +44:56:17.4
05:52:08.42 +49:39:12.6
########### Completed Aur-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
05:55:50.61 +46:34:58.5
06:06:53.96 +48:50:11.6
05:53:23.62 +43:27:34.5
05:36:44.15 +43:04:49.3
05:56:05.28 +44:35:31.2
05:56:52.39 +43:51:21.8
05:53:04.86 +46:58:02.5
05:51:27.67 +45:11:26.4
05:56:14.85 +48:35:48.1
05:37:29.65 +43:17:37.0
05:52:59.33 +46:57:31.1
05:40:29.48 +46:12:11.1
05:35:49.54 +43:04:58.2
06:13:09.47 +45:05:09.4
05:35:09.96 +46:58:05.6
06:35:49.95 +48:37:47.4
06:02:14.37 +47:47:00.4
06:16:04.85 +43:18:56.4
05:56:59.32 +46:26:55.8
06:08:44.09 +48:20:44.4
05:48:13.23 +42:46:42.2
06:00:35.20 +48:33:25.3
05:54:07.84 +41:46:23.6
06:25:08.20 +42:30:49.3
06:31:57.28 +45:00:41.7
06:20:12.71 +43:38:54.5
05:58:32.71 +44:49:13.1
06:12:10.23 +50:14:53.5
06:26:19.92 +41:59:08.5
05:53:17.73 +43:17:15.4
06:25:57.22 +43:06:04.9
06:13:29.56 +41:58:05.4
05:54:13.39 +47:53:37.4
05:59:58.97 +43:51:29.8
06:13:33.54 +48:03:16.7
06:02:32.06 +48:11:24.9
05:57:45.30 +45:54:52.2
06:26:29.60 +49:54:11.0
05:57:11.25 +42:50:25.8
05:37:19.39 +44:51:38.5
05:57:07.90 +43:07:28.5
06:00:04.32 +45:58:32.6
05:37:44.70 +42:36:38.6
05:42:53.55 +47:11:05.6
05:36:40.84 +50:02:54.9
06:08:04.94 +45:02:04.4
05:39:18.97 +44:01:55.4
05:38:59.94 +47:35:32.1
05:41:02.57 +46:20:39.0
05:46:32.87 +45:16:05.6
05:37:52.40 +43:02:35.5
05:52:57.86 +44:33:10.5
05:50:28.69 +44:11:34.4
06:01:02.32 +47:22:14.5
05:49:08.62 +44:09:11.8
06:10:45.00 +48:16:56.3
06:04:15.55 +46:54:36.7
05:52:55.17 +42:18:28.1
05:54:16.08 +41:58:03.4
05:44:02.82 +45:51:12.0
05:42:06.12 +41:56:49.5
05:50:56.43 +44:56:17.4
05:52:08.42 +49:39:12.6
###################################################################################
05:55:50.61 +46:34:58.5 -- not an asteroid (will add it to exclusion list)
06:06:53.96 +48:50:11.6 -- not an asteroid (will add it to exclusion list)
05:53:23.62 +43:27:34.5 -- not an asteroid (will add it to exclusion list)
05:36:44.15 +43:04:49.3 -- not an asteroid (will add it to exclusion list)
05:56:05.28 +44:35:31.2 -- not an asteroid (will add it to exclusion list)
05:56:52.39 +43:51:21.8 -- not an asteroid (will add it to exclusion list)
05:53:04.86 +46:58:02.5 -- not an asteroid (will add it to exclusion list)
05:51:27.67 +45:11:26.4 -- not an asteroid (will add it to exclusion list)
05:56:14.85 +48:35:48.1 -- not an asteroid (will add it to exclusion list)
05:37:29.65 +43:17:37.0 -- not an asteroid (will add it to exclusion list)
05:52:59.33 +46:57:31.1 -- not an asteroid (will add it to exclusion list)
05:40:29.48 +46:12:11.1 -- not an asteroid (will add it to exclusion list)
05:35:49.54 +43:04:58.2 -- not an asteroid (will add it to exclusion list)
06:13:09.47 +45:05:09.4 -- not an asteroid (will add it to exclusion list)
05:35:09.96 +46:58:05.6 -- not an asteroid (will add it to exclusion list)
06:35:49.95 +48:37:47.4 -- not an asteroid (will add it to exclusion list)
06:02:14.37 +47:47:00.4 -- not an asteroid (will add it to exclusion list)
06:16:04.85 +43:18:56.4 -- not an asteroid (will add it to exclusion list)
05:56:59.32 +46:26:55.8 -- not an asteroid (will add it to exclusion list)
06:08:44.09 +48:20:44.4 -- not an asteroid (will add it to exclusion list)
05:48:13.23 +42:46:42.2 -- not an asteroid (will add it to exclusion list)
06:00:35.20 +48:33:25.3 -- not an asteroid (will add it to exclusion list)
05:54:07.84 +41:46:23.6 -- not an asteroid (will add it to exclusion list)
06:25:08.20 +42:30:49.3 -- not an asteroid (will add it to exclusion list)
06:31:57.28 +45:00:41.7 -- not an asteroid (will add it to exclusion list)
06:20:12.71 +43:38:54.5 -- not an asteroid (will add it to exclusion list)
05:58:32.71 +44:49:13.1 -- not an asteroid (will add it to exclusion list)
06:12:10.23 +50:14:53.5 -- not an asteroid (will add it to exclusion list)
06:26:19.92 +41:59:08.5 -- not an asteroid (will add it to exclusion list)
05:53:17.73 +43:17:15.4 -- not an asteroid (will add it to exclusion list)
06:25:57.22 +43:06:04.9 -- not an asteroid (will add it to exclusion list)
06:13:29.56 +41:58:05.4 -- not an asteroid (will add it to exclusion list)
05:54:13.39 +47:53:37.4 -- not an asteroid (will add it to exclusion list)
05:59:58.97 +43:51:29.8 -- not an asteroid (will add it to exclusion list)
06:13:33.54 +48:03:16.7 -- not an asteroid (will add it to exclusion list)
06:02:32.06 +48:11:24.9 -- not an asteroid (will add it to exclusion list)
05:57:45.30 +45:54:52.2 -- not an asteroid (will add it to exclusion list)
06:26:29.60 +49:54:11.0 -- not an asteroid (will add it to exclusion list)
05:57:11.25 +42:50:25.8 -- not an asteroid (will add it to exclusion list)
05:37:19.39 +44:51:38.5 -- not an asteroid (will add it to exclusion list)
05:57:07.90 +43:07:28.5 -- not an asteroid (will add it to exclusion list)
06:00:04.32 +45:58:32.6 -- not an asteroid (will add it to exclusion list)
05:37:44.70 +42:36:38.6 -- not an asteroid (will add it to exclusion list)
05:42:53.55 +47:11:05.6 -- not an asteroid (will add it to exclusion list)
05:36:40.84 +50:02:54.9 -- not an asteroid (will add it to exclusion list)
06:08:04.94 +45:02:04.4 -- not an asteroid (will add it to exclusion list)
05:39:18.97 +44:01:55.4 -- not an asteroid (will add it to exclusion list)
05:38:59.94 +47:35:32.1 -- not an asteroid (will add it to exclusion list)
05:41:02.57 +46:20:39.0 -- not an asteroid (will add it to exclusion list)
05:46:32.87 +45:16:05.6 -- not an asteroid (will add it to exclusion list)
05:37:52.40 +43:02:35.5 -- not an asteroid (will add it to exclusion list)
05:52:57.86 +44:33:10.5 -- not an asteroid (will add it to exclusion list)
05:50:28.69 +44:11:34.4 -- not an asteroid (will add it to exclusion list)
06:01:02.32 +47:22:14.5 -- not an asteroid (will add it to exclusion list)
05:49:08.62 +44:09:11.8 -- not an asteroid (will add it to exclusion list)
06:10:45.00 +48:16:56.3 -- not an asteroid (will add it to exclusion list)
06:04:15.55 +46:54:36.7 -- not an asteroid (will add it to exclusion list)
05:52:55.17 +42:18:28.1 -- not an asteroid (will add it to exclusion list)
05:54:16.08 +41:58:03.4 -- not an asteroid (will add it to exclusion list)
05:44:02.82 +45:51:12.0 -- not an asteroid (will add it to exclusion list)
05:42:06.12 +41:56:49.5 -- not an asteroid (will add it to exclusion list)
05:50:56.43 +44:56:17.4 -- not an asteroid (will add it to exclusion list)
05:52:08.42 +49:39:12.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:35:09.96 +46:58:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:49.54 +43:04:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.84 +50:02:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:44.15 +43:04:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.39 +44:51:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:29.65 +43:17:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:44.70 +42:36:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.40 +43:02:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:59.94 +47:35:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:18.97 +44:01:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:29.48 +46:12:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:02.57 +46:20:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:06.12 +41:56:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:53.55 +47:11:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:02.82 +45:51:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:32.87 +45:16:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:13.23 +42:46:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:08.62 +44:09:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.69 +44:11:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:56.43 +44:56:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:27.67 +45:11:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:08.42 +49:39:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:55.17 +42:18:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:57.86 +44:33:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:59.33 +46:57:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.86 +46:58:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:17.73 +43:17:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:23.62 +43:27:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:07.84 +41:46:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:13.39 +47:53:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:16.08 +41:58:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:50.61 +46:34:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:05.28 +44:35:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:14.85 +48:35:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:52.39 +43:51:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:59.32 +46:26:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:07.90 +43:07:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.25 +42:50:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:45.30 +45:54:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:32.71 +44:49:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:58.97 +43:51:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:04.32 +45:58:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:35.20 +48:33:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:02.32 +47:22:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.37 +47:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.06 +48:11:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.55 +46:54:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:06:53.96 +48:50:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:04.94 +45:02:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:44.09 +48:20:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.00 +48:16:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.23 +50:14:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:09.47 +45:05:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.56 +41:58:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:33.54 +48:03:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:04.85 +43:18:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:12.71 +43:38:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:08.20 +42:30:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:57.22 +43:06:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.92 +41:59:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.60 +49:54:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:57.28 +45:00:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:49.95 +48:37:47.4 -- 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)
05:35:09.96 +46:58:05.6 -- a known variable star
05:35:49.54 +43:04:58.2 -- a known variable star
05:36:40.84 +50:02:54.9 -- not a known variable star
05:36:44.15 +43:04:49.3 -- not a known variable star
05:37:19.39 +44:51:38.5 -- not a known variable star
05:37:29.65 +43:17:37.0 -- not a known variable star
05:37:44.70 +42:36:38.6 -- a known variable star
05:37:52.40 +43:02:35.5 -- not a known variable star
05:38:59.94 +47:35:32.1 -- not a known variable star
05:39:18.97 +44:01:55.4 -- not a known variable star
05:40:29.48 +46:12:11.1 -- not a known variable star
05:41:02.57 +46:20:39.0 -- not a known variable star
05:42:06.12 +41:56:49.5 -- not a known variable star
05:42:53.55 +47:11:05.6 -- not a known variable star
05:44:02.82 +45:51:12.0 -- not a known variable star
05:46:32.87 +45:16:05.6 -- not a known variable star
05:48:13.23 +42:46:42.2 -- not a known variable star
05:49:08.62 +44:09:11.8 -- not a known variable star
05:50:28.69 +44:11:34.4 -- a known variable star
05:50:56.43 +44:56:17.4 -- not a known variable star
05:51:27.67 +45:11:26.4 -- a known variable star
05:52:08.42 +49:39:12.6 -- not a known variable star
05:52:55.17 +42:18:28.1 -- not a known variable star
05:52:57.86 +44:33:10.5 -- a known variable star
05:52:59.33 +46:57:31.1 -- not a known variable star
05:53:04.86 +46:58:02.5 -- not a known variable star
05:53:17.73 +43:17:15.4 -- not a known variable star
05:53:23.62 +43:27:34.5 -- not a known variable star
05:54:07.84 +41:46:23.6 -- a known variable star
05:54:13.39 +47:53:37.4 -- not a known variable star
05:54:16.08 +41:58:03.4 -- not a known variable star
05:55:50.61 +46:34:58.5 -- not a known variable star
05:56:05.28 +44:35:31.2 -- not a known variable star
05:56:14.85 +48:35:48.1 -- not a known variable star
05:56:52.39 +43:51:21.8 -- not a known variable star
05:56:59.32 +46:26:55.8 -- not a known variable star
05:57:07.90 +43:07:28.5 -- not a known variable star
05:57:11.25 +42:50:25.8 -- not a known variable star
05:57:45.30 +45:54:52.2 -- not a known variable star
05:58:32.71 +44:49:13.1 -- not a known variable star
05:59:58.97 +43:51:29.8 -- not a known variable star
06:00:04.32 +45:58:32.6 -- not a known variable star
06:00:35.20 +48:33:25.3 -- not a known variable star
06:01:02.32 +47:22:14.5 -- not a known variable star
06:02:14.37 +47:47:00.4 -- a known variable star
06:02:32.06 +48:11:24.9 -- not a known variable star
06:04:15.55 +46:54:36.7 -- not a known variable star
06:06:53.96 +48:50:11.6 -- a known variable star
06:08:04.94 +45:02:04.4 -- not a known variable star
06:08:44.09 +48:20:44.4 -- not a known variable star
06:10:45.00 +48:16:56.3 -- not a known variable star
06:12:10.23 +50:14:53.5 -- not a known variable star
06:13:09.47 +45:05:09.4 -- not a known variable star
06:13:29.56 +41:58:05.4 -- not a known variable star
06:13:33.54 +48:03:16.7 -- not a known variable star
06:16:04.85 +43:18:56.4 -- a known variable star
06:20:12.71 +43:38:54.5 -- a known variable star
06:25:08.20 +42:30:49.3 -- not a known variable star
06:25:57.22 +43:06:04.9 -- a known variable star
06:26:19.92 +41:59:08.5 -- not a known variable star
06:26:29.60 +49:54:11.0 -- not a known variable star
06:31:57.28 +45:00:41.7 -- not a known variable star
06:35:49.95 +48:37:47.4 -- not a known variable star
Found 51 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
63 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 63 (excluding asteroids and hot pixels, 51 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)2461144.63846649 -observatory V36
23:57:36.42 -03:03:05.9 Mercury (0.1mag)
02:59:34.06 +17:08:51.2 Venus (-3.9mag)
00:12:33.08 +00:16:57.3 Mars (1.2mag)
07:11:48.17 +22:47:35.0 Jupiter (-2.1mag)
00:28:20.99 +00:43:47.6 Saturn (0.9mag)
03:47:18.47 +19:46:13.7 Uranus (5.8mag)
00:10:35.75 -00:16:54.8 Neptune (7.8mag)
20:33:40.20 -22:52:31.4 Pluto (14.5mag)
22:44:14.36 -08:08:11.8 Moon (-9.2mag)
-rw-r--r-- 1 apache apache 361 Apr 13 22:28 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461144.63846649:
07:11:43.89 +22:47:45.8 Io (5.8mag)
07:11:47.59 +22:47:33.1 Europa (5.9mag)
07:11:56.16 +22:47:25.1 Ganymede (5.3mag)
07:12:14.21 +22:46:48.9 Callisto (6.6mag)
07:15:13.23 +22:36:05.1 Himalia (15.3mag)
07:11:45.02 +22:47:40.3 Thebe (16.2mag)
07:15:22.18 +23:06:07.6 Elara (17.3mag)
07:10:33.45 +23:28:33.8 Pasiphae (17.4mag)
07:20:10.33 +22:45:25.2 Carme (18.5mag)
00:28:29.09 +00:44:03.5 Titan (8.8mag)
00:28:23.31 +00:44:01.1 Rhea (10.1mag)
00:28:04.37 +00:44:14.8 Iapetus (11.5mag)
00:28:34.35 +00:43:56.3 Hyperion (14.8mag)
00:29:59.36 +00:52:47.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 22:29 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461144.63846649:
15:30:00.63 -14:54:22.1 JWST
16:59:03.73 +44:39:49.1 Chandra
07:54:10.69 -35:18:23.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 22:28 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461144.63846649 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:51:13.17 -28:40:13.9 13.9mag P/2010 H2 (Vales)
05:05:24.48 -69:45:02.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:02.98 +31:25:29.5 17.2mag C/2017 K2 (PANSTARRS)
17:30:36.44 +10:19:36.3 17.6mag C/2021 G2 (ATLAS)
23:09:43.34 +29:09:20.5 17.1mag C/2022 E2 (ATLAS)
04:27:04.25 +25:59:16.0 16.0mag C/2022 N2 (PANSTARRS)
09:03:02.06 +32:00:19.8 16.2mag C/2022 QE78 (ATLAS)
08:30:47.83 -00:21:04.1 17.3mag C/2022 R6 (PANSTARRS)
18:54:09.73 +18:22:32.9 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:16.20 -11:32:55.6 17.5mag P/2023 B1 (PANSTARRS)
09:08:30.79 -12:10:56.9 17.6mag C/2023 F3 (ATLAS)
21:52:19.49 +62:47:53.3 17.5mag C/2023 H5 (Lemmon)
19:20:46.59 -03:42:10.2 14.2mag C/2023 R1 (PANSTARRS)
21:35:56.43 +85:39:15.6 17.8mag C/2023 X2 (Lemmon)
06:17:03.45 +63:31:19.1 17.1mag C/2024 A1 (ATLAS)
05:09:15.27 +17:40:37.9 10.9mag C/2024 E1 (Wierzchos)
16:20:27.78 +06:05:06.8 17.4mag C/2024 G6 (ATLAS)
20:20:16.70 +14:46:13.3 14.6mag C/2024 J3 (ATLAS)
03:24:42.03 -22:40:11.5 16.4mag C/2024 T5 (ATLAS)
05:15:08.32 +45:45:20.3 17.7mag C/2025 J1 (Borisov)
13:46:34.51 +44:13:52.5 15.1mag C/2025 L1 (ATLAS)
03:22:20.71 -25:55:22.0 17.8mag C/2025 Q3 (ATLAS)
23:28:31.71 +19:09:00.0 8.8mag C/2025 R3 (PANSTARRS)
12:54:55.58 +02:53:56.7 17.4mag C/2025 Y1 (ATLAS)
03:11:52.48 +02:50:20.3 12.7mag C/2026 A1 (MAPS)
23:54:16.66 +36:52:22.7 14.5mag C/2026 B2 (Sun-Gao)
18:39:18.65 -09:49:06.3 11.9mag 10P/Tempel
15:02:49.26 +03:24:01.3 13.8mag 24P/Schaumasse
11:03:18.47 -01:35:11.7 15.7mag 29P/Schwassmann-Wachmann
18:00:23.65 -09:40:44.7 17.9mag 40P/Vaisala
10:37:39.74 -04:14:54.1 16.9mag 43P/Wolf-Harrington
01:45:47.50 +17:10:12.1 17.2mag 47P/Ashbrook-Jackson
07:07:20.43 +37:24:44.2 17.0mag 63P/Wild
23:26:40.66 -11:40:29.8 15.7mag 65P/Gunn
03:58:17.16 +20:36:44.3 15.9mag 76P/West-Kohoutek-Ikemura
01:01:27.65 +07:51:45.3 14.3mag 78P/Gehrels
22:57:20.96 -09:56:29.7 14.6mag 88P/Howell
02:05:08.41 +20:08:40.3 15.1mag 93P/Lovas
04:51:18.29 +32:11:16.6 16.2mag 123P/West-Hartley
08:26:11.60 +39:13:13.4 16.2mag 124P/Mrkos
02:30:20.41 +14:09:43.4 16.4mag 128P/Shoemaker-Holt
02:43:53.12 +14:15:55.4 17.5mag 131P/Mueller
01:16:24.28 +12:35:22.5 10.7mag 141P/Machholz
01:25:35.31 +04:10:29.7 10.7mag 141P-A/Machholz
00:11:47.38 +00:09:15.5 13.0mag 141P-D/Machholz
01:55:45.29 +05:55:39.6 17.8mag 141P-I/Machholz
00:57:11.17 -02:27:42.8 15.1mag 162P/SidingSpring
10:29:06.37 +30:57:36.2 18.0mag 164P/Christensen
06:33:05.31 +24:18:02.3 18.0mag 198P/ODAS
14:54:44.72 -00:15:45.5 17.6mag 210P/Christensen
21:33:25.67 -11:53:51.2 17.6mag 218P/LINEAR
17:16:04.11 -14:09:22.8 16.1mag 235P/LINEAR
05:30:27.98 +34:33:21.6 16.7mag 240P/NEAT
07:37:35.30 -05:22:11.4 17.7mag 242P/Spahr
22:12:15.28 -21:28:20.0 17.9mag 260P/McNaught
15:43:21.65 +06:52:01.4 17.5mag 391P/Kowalski
07:33:29.42 +21:21:35.6 17.7mag 450P/LONEOS
05:33:09.63 +45:08:30.5 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 22:28 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
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
-rw-r--r-- 1 apache apache 5.8K Apr 13 22:28 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 13 22:28 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:46:07.094 +07:14:13.61 AT 2026ive 2026-04-08.15 19.9446
09:29:29.340 -01:21:08.51 AT 2026ivd 2026-04-05.15 19.4593
09:53:27.521 +16:01:50.20 AT 2026ivc 2026-04-07.17 20.1328
10:57:27.283 +18:19:29.99 AT 2026ivb 2026-04-07.87 19.71
12:50:08.105 +01:17:40.78 AT 2026iva 2026-04-07.89 19.96
10:38:31.370 -04:47:42.62 AT 2026iuz 2026-04-07.85 18.9
13:03:44.252 +20:35:06.20 AT 2026iuy 2026-04-06.96 19.7
13:53:33.216 -46:24:12.81 AT 2026iux 2026-04-07.63 19.83
20:29:30.119 -10:56:33.33 AT 2026iuw 2026-03-29.79 19.55
13:31:30.960 -32:00:09.92 AT 2026iuv 2026-04-07.60 18.91
14:00:56.468 -25:06:29.29 AT 2026iuu 2026-04-07.35 18.482
13:27:25.132 +09:30:53.72 AT 2026iut 2026-04-05.33 19.4971
13:57:28.106 -31:36:18.49 AT 2026ius 2026-04-07.61 19.27
09:54:32.050 -01:17:25.84 SN 2026iur 2026-04-07.01 15.9
14:24:08.131 +22:56:14.71 AT 2026iuq 2026-04-07.38 19.91
10:07:28.221 -17:12:04.00 AT 2026iup 2026-04-05.31 20.26
16:21:33.361 +42:39:39.49 AT 2026iuo 2026-04-02.59 20.72
11:27:41.500 -35:48:12.21 AT 2026iun 2026-03-30.51 19.56
13:57:31.503 -10:38:39.68 AT 2026ium 2026-03-29.71 19.95
19:51:44.150 +31:28:49.50 AT 2026iul 2026-04-07.40 15.7
-rw-r--r-- 1 apache apache 30K Apr 13 22:28 tns_transients_list.txt
