This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.46,0.05,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
target 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.9379+44.9337,2461138.7235,13.16,0.05,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 J084.9379+44.9337 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194428260345596160,2461138.7235,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194428260345596160 20260408.2235 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3290+41.8878,2461138.7235,12.88,0.05,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 J093.3290+41.8878 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.80,0.05,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 20260408.2235 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 958672228438497152,2461138.7235,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 958672228438497152 20260408.2235 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.4229+42.7600,2461138.7235,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.4229+42.7600 20260408.2235 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192716728762870272,2461138.7235,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192716728762870272 20260408.2235 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9926+46.7105,2461138.7235,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.9926+46.7105 20260408.2235 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.31,0.05,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 20260408.2235 12.31CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J06094478+4704276,2461138.7235,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J06094478+4704276 20260408.2235 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192393648438331136,2461138.7235,12.47,0.05,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 192393648438331136 20260408.2235 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 960874520165473536,2461138.7235,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 960874520165473536 20260408.2235 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9474+42.5087,2461138.7235,12.55,0.05,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
ATO J088.9474+42.5087 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5514+42.8423,2461138.7235,12.80,0.05,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 J089.5514+42.8423 20260408.2235 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.88,0.05,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 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3774+41.9686,2461138.7235,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3774+41.9686 20260408.2235 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461138.7235,12.94,0.05,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
ATO J090.6351+48.1884 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1509+45.4814,2461138.7235,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1509+45.4814 20260408.2235 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.7693+49.1987,2461138.7235,13.10,0.05,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 J095.7693+49.1987 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461138.7235,13.05,0.05,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 197388553666998656 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461138.7235,13.04,0.05,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 196552271996570368 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.20,0.05,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
target 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196839661143429120,2461138.7235,13.16,0.05,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
Gaia DR3 196839661143429120 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.10,0.05,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
target 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461138.7235,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196552271996570368 20260408.2235 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461138.7235,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2776+47.3006 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192463089469495040,2461138.7235,13.13,0.05,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
Gaia DR3 192463089469495040 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197288807346758784,2461138.7235,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197288807346758784 20260408.2235 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.8798+49.8178,2461138.7235,13.21,0.05,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
ATO J084.8798+49.8178 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.4431+44.2946,2461138.7235,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.4431+44.2946 20260408.2235 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196540181664371200,2461138.7235,13.27,0.05,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
Gaia DR3 196540181664371200 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.26,0.05,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 20260408.2235 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2314+46.6988,2461138.7235,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2314+46.6988 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0747+46.9169,2461138.7235,13.27,0.05,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 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7235,13.27,0.05,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
VARIABLE_NAME 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210103654024515072,2461138.7235,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210103654024515072 20260408.2235 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 962218531395116928,2461138.7235,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 962218531395116928 20260408.2235 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.3439+46.5769,2461138.7235,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.3439+46.5769 20260408.2235 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.6159+43.7708,2461138.7235,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.6159+43.7708 20260408.2235 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210216624548997760,2461138.7235,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210216624548997760 20260408.2235 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.6178+44.7898,2461138.7235,13.47,0.05,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 J088.6178+44.7898 20260408.2235 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197829737003759872,2461138.7235,13.53,0.05,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
Gaia DR3 197829737003759872 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.52,0.05,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 20260408.2235 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.6565+44.1335,2461138.7235,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.6565+44.1335 20260408.2235 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7235,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2235 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461138.72372831 08.04.2026 05:22:00.126 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
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: 5 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): 16330
Objects passed selection criteria: 16305
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: 14496.8
Average stars matched: 14142.8 (97.5581 %)
Memory usage VmPeak: 122832 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 00:25:51 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461138.72372831 08.04.2026 05:22:00.126 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 393
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: 55 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): 123545
Objects passed selection criteria: 123221
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 112415
Average stars matched: 108757 (96.746 %)
Memory usage VmPeak: 2353620 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 00:27:46 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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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: 2461138.72321875
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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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 06:00:01.360 +46:00:20.01
Angular distance between the image centers 0.0394 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 06:00:01.244 +46:00:15.57
Angular distance between the image centers 0.0392 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 06:00:01.360 +46:00:20.01
Second-epoch second image center 06:00:01.244 +46:00:15.57
Angular distance between the image centers 0.00128 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00128 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.I6jWB3wHKQ
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.MNQ3Aw1Q8K
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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits &> /tmp/tmp.pVp3m5gxVj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits &> /tmp/tmp.lFtBEzvLNz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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 7 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
2.5 pix fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
2.5 pix fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.I6jWB3wHKQ (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.MNQ3Aw1Q8K (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.pVp3m5gxVj (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1017, passed=16675
Got 16675 stars (including 15635 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 16675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 16290 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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 16290 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 16290 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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.lFtBEzvLNz (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=994, passed=16573
Got 16573 stars (including 15560 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 16573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 16166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 16166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 16166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31358.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31048_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31048_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:48.09 +41:57:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.074 194422522269714816 084.20064345506 +41.95441735956 10.9821 10.0230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31154_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31154_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:59:43.45 +44:59:09.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:14:59.02 +46:47:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31181_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31181_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:22.94 +46:49:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31270_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31270_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:45:42.91 +43:37:26.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31346_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31346_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:55:20.91 +43:16:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.955 193310160099657216 088.83737940998 +43.28199553885 12.1323 11.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31358_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 31358_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:28:45.88 +48:34:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.466 967547868550025216 097.19110438442 +48.57701626020 12.2587 11.7628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 2s
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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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 06:00:01.360 +46:00:20.01
Angular distance between the image centers 0.0394 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 06:00:01.244 +46:00:15.57
Angular distance between the image centers 0.0392 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 06:00:01.360 +46:00:20.01
Second-epoch second image center 06:00:01.244 +46:00:15.57
Angular distance between the image centers 0.00128 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00128 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.7VIJJpDntu
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.j9dxJL0f7H
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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits &> /tmp/tmp.rAq6oBvPQ1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits &> /tmp/tmp.Co4lux2sAj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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 285 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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7VIJJpDntu (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.j9dxJL0f7H (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.rAq6oBvPQ1 (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=10415, passed=116631
Got 116631 stars (including 106096 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat
util/solve_plate_with_UCAC5 got 116631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 114957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 114960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 114960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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.Co4lux2sAj (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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=10454, passed=115863
Got 115863 stars (including 105291 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 115863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 113696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 113696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 113694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/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_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-21-16_20.00sec_-5.00C_LIGHT_0025.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.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_2026-04-08_CI_Aur-02-Q2b1x1_002333_TTUQ2b1x1_16452_eqA87fNc/wcs_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out192137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out192109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194214.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194666.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 81s
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: 34s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192109_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192109_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192118_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192118_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192137_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192137_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:41:56.80 +41:50:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.813 192860322404512256 085.48696887357 +41.83379326049 14.5783 13.9830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192148_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192148_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 192150_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192150_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:17.19 +47:02:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192156_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192156_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192157_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192157_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:45:23.77 +41:43:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.257 192749817188338176 086.34857635676 +41.73273222407 14.0805 13.2517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192163_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192163_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192169_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192169_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:14:16.81 +44:50:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.906 962437510303270272 093.56998254246 +44.83722410185 14.4415 13.7845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192176_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192176_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:35.94 +46:53:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.470 209815444538865408 085.15044753050 +46.89347890104 12.1234 10.4153 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192179_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192179_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:25.02 +45:43:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.035 209501087293588224 084.35462223877 +45.72979338931 14.0253 13.1241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192182_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192182_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192183_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192183_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192187_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192187_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192188_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192188_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:00.27 +42:27:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.378 194494368482144896 084.25126338216 +42.45554787083 13.8924 13.0809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192200_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192200_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:50:32.96 +42:15:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192204_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192204_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:30.43 +46:11:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.787 209537813557420800 085.12731334874 +46.19873181443 13.9698 13.4266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192205_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192205_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:03.94 +44:42:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.646 962801345573631744 092.76641967986 +44.71092930293 14.0950 13.6515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192209_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192209_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:05:26.87 +42:40:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192211_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:24:03.89 +44:40:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.827 959256898041674880 096.01653084857 +44.67501473517 13.9280 13.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192212_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192212_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:23:15.22 +43:57:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.454 962119270406749440 095.81350455544 +43.96249806494 13.9474 13.3886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192214_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192214_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192217_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192217_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192225_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192234_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192234_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:26:53.33 +43:56:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192235_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:56:29.59 +45:53:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.738 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192240_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192240_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:36:57.80 +44:14:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192241_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192241_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:17:15.73 +41:56:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.675 960066757075630848 094.31559533137 +41.94393329122 13.2868 12.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192245_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192245_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192246_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192246_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:12:49.22 +42:16:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192247_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192247_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:46.88 +41:49:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.807 194407640206192896 084.19600591223 +41.82222203813 13.4697 13.2053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192251_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192251_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192252_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192252_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192255_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192255_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:16:42.98 +44:42:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.975 962379987803965568 094.17937221668 +44.71614908613 13.4420 12.7072 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 192256_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192256_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:38:24.22 +42:05:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192260_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192260_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:19:25.28 +44:38:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.751 962202214814317312 094.85547961849 +44.64084749790 13.1782 12.5035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192261_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192261_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192263_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192263_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:42:01.62 +46:28:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192264_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192264_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:31:57.22 +45:00:43.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 192265_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192265_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:13.06 +47:02:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192266_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192266_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:31:06.81 +48:10:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192267_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192267_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:01:39.43 +45:44:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.406 963145561432116224 090.41445434671 +45.73787381455 13.0287 12.5054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192271_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192271_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:29:14.81 +41:54:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192273_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192273_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:41:57.58 +44:20:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.914 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192275_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192275_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:20:12.73 +43:38:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 1.324 961773920675999104 095.05336462401 +43.64875630381 12.9196 12.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192276_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192276_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:23.49 +49:53:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192277_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192281_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192281_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:54:42.23 +43:39:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.798 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192282_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192282_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:45.97 +43:34:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192284_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192284_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:48.09 +41:57:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.22, MAG_FAINT_SEARCH_LIMIT=11.20)GAIADR2_OUTPUT=# 1.074 194422522269714816 084.20064345506 +41.95441735956 10.9821 10.0230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192405_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192405_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:22.95 +46:49:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192419_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192419_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192519_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192519_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192536_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192536_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192540_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192540_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192572_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192572_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:34.52 +48:44:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192673_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192673_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:51:47.60 +48:44:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192675_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192675_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192685_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192685_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:46:26.50 +47:55:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192700_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192700_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192730_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192730_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192737_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192737_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:06:21.22 +48:46:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192742_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192742_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:19:04.21 +47:21:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192817_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192817_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192846_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192846_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192899_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192899_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:13:46.67 +44:43:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192901_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192901_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192907_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192907_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192908_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192908_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:02.81 +50:02:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192909_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192909_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:39:07.58 +44:53:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192931_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192931_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192937_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192937_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:05:50.21 +44:39:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192965_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 192965_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 192990_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192990_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192992_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192992_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 192995_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 192995_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:34:37.46 +45:55:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193001_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193001_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193015_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193015_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:48:04.07 +43:19:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193028_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193028_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:02.41 +49:49:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193037_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193037_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193049_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193049_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193055_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193055_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193066_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193066_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193077_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193077_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193086_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193086_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:46.05 +45:53:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193104_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193104_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193105_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193105_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193106_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193106_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:03:13.58 +42:56:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193107_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193107_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193117_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193117_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193141_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193141_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193142_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193142_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193147_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193147_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193164_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193164_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:32.57 +43:42:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193165_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:00.98 +47:29:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193176_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193176_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:47:45.28 +50:03:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193181_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193181_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193185_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193185_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193202_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193202_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193211_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193211_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193219_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193219_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:17:34.58 +46:23:46.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193231_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193231_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:53:12.01 +45:24:23.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193238_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193238_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193244_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193244_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193253_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193253_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:49.30 +45:03:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.082 963207786918929408 092.95523434237 +45.05495257659 13.4231 12.7204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193255_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193255_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193263_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193263_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193264_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193264_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:52:03.70 +49:32:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193270_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193270_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:14.23 +50:00:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193285_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193285_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:01:04.64 +50:00:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193306_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193306_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:08:02.24 +46:40:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.220 963435214026488704 092.00979468381 +46.68289863325 13.5967 13.1319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193309_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193309_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193328_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193328_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:43:06.51 +44:51:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193329_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193329_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:44.69 +44:40:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.368 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193339_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193339_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193348_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193348_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193356_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193356_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193361_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193361_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:38:24.36 +42:59:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193368_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193368_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193380_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193380_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:25:57.49 +43:06:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.568 959056340249435648 096.49003720301 +43.10182569324 13.6518 12.9992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193382_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193382_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:56:30.93 +46:14:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.884 197751809117411712 089.12908358575 +46.24714326154 13.6175 12.8385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193394_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193394_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:56:51.32 +48:55:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.608 210461201461752192 089.21406534870 +48.93146143301 13.6447 13.0132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193398_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193398_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:44:48.27 +48:58:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193408_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193408_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193414_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193414_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193426_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193426_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:00:13.89 +47:43:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193441_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193441_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193458_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193458_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:38:46.48 +46:04:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193481_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193481_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:01:16.77 +47:35:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193497_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193497_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193499_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193499_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:31.24 +47:51:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.327 210289196612409472 087.38044179706 +47.86209697171 13.6067 12.8112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193508_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193508_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193513_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193513_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193517_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193517_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:10:01.84 +47:39:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.870 969468887162852736 092.50786637866 +47.65128419673 13.7413 13.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193518_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193518_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:44:39.90 +43:57:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193523_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193523_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193544_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193544_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:13:42.08 +45:31:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.738 962485506560815104 093.42562997977 +45.51967529314 11.4649 9.7766 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193548_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193548_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:06.31 +45:12:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193552_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193552_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:38:50.48 +49:49:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193561_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193561_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193562_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193562_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193579_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193579_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193581_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193581_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193582_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193582_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:08:18.90 +41:46:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193584_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193584_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:38:22.08 +42:59:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193597_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193597_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193607_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193607_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193621_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193621_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:46:39.69 +43:21:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.504 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193631_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193631_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:20:02.76 +46:37:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.638 968511624851868672 095.01136623934 +46.62745956761 13.9610 13.3520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193633_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193633_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193639_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193639_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193645_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193645_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193650_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193650_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193671_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193671_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193672_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193672_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:48:23.32 +49:46:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.791 211485637061247744 087.09740055049 +49.78256265660 13.8223 13.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193674_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193674_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193684_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193684_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193688_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193688_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193689_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193689_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193696_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193696_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193710_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193710_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:03:43.54 +50:12:55.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193717_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193717_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193719_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193719_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:42:50.74 +48:07:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.648 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193736_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193736_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193744_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193744_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:45.40 +45:54:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.552 196999777523639936 089.43970142505 +45.91480103623 13.9429 13.4194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193746_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193746_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:48:44.69 +49:34:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.800 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193748_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193748_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193761_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193761_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:18.68 +47:12:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.924 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193769_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193769_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:43:56.69 +47:43:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.632 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193780_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193780_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193786_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193786_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:44.66 +42:36:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.997 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193789_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193789_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:52:21.14 +42:50:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193791_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193791_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193795_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193795_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193814_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193814_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:39:18.50 +44:01:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193817_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193817_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:24.77 +49:14:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.893 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193818_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193818_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:22:29.82 +44:29:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.526 962230007546590208 095.62484427373 +44.49039250040 13.9307 13.4207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193826_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193826_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193836_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193836_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193840_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193840_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:27.91 +47:51:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.410 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193846_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193846_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:57.46 +42:25:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193851_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193851_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:03:20.98 +42:41:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.813 960875035561541376 090.83923379420 +42.69689639166 13.9565 13.4004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193853_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193853_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193858_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193858_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:11:51.76 +45:03:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.283 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193870_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193870_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193873_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193873_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:40:59.49 +46:21:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193884_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193884_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193899_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193899_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193919_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193919_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193925_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193925_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193931_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193931_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193938_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193938_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193940_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193940_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 193943_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193943_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193960_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193960_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193964_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193964_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193967_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193967_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193970_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193970_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:53:28.98 +46:52:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.278 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193972_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193972_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:25:45.50 +45:22:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193980_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 193980_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 193982_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193982_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:59:59.04 +43:51:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.059 193350945108672256 089.99625078820 +43.85828750162 14.0064 13.4492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193987_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 193987_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:49:25.44 +42:20:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.960 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194001_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194001_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:53.16 +46:05:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194002_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194002_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194023_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194023_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194030_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194030_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194044_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194044_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:36:07.16 +47:47:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.980 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194054_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194054_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:58:09.59 +48:37:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.718 210251469618523520 089.54055114472 +48.62003298825 14.3909 13.8430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194058_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194058_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194059_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194059_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194060_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194060_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194084_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194084_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:17:15.36 +42:06:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194088_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194088_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194096_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194096_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194117_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194117_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194121_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194121_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194128_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194128_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:53:58.31 +42:30:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.627 192386845210042624 088.49355776279 +42.50729470844 14.1038 13.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194129_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194129_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:12:20.01 +50:12:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194135_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194135_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194148_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194148_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194159_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194159_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194160_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194160_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194173_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194173_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194174_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194174_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194178_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194178_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194189_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194189_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194199_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194199_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194205_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194205_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194214_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194214_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194250_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194250_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194268_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194268_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194304_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194304_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:03:02.61 +46:43:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194330_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194330_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:10:00.12 +45:32:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.149 963235820168851712 092.50109436752 +45.54496087176 14.4482 13.9808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194345_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194345_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194347_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194347_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194351_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194351_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194352_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194352_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:54:21.60 +42:55:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.215 193251645465407488 088.59009184359 +42.91869191532 14.2168 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194382_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194382_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194383_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194383_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194405_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194405_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194409_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194409_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194419_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194419_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194451_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194451_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:00:27.28 +42:54:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.432 960919050386214528 090.11419266104 +42.91073825498 14.5959 13.7863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194455_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194455_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194473_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194473_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194484_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194484_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194489_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194489_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194496_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194496_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194497_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194497_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:44:47.08 +46:28:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.029 209612206687131136 086.19689831834 +46.47272458834 14.4861 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194511_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194511_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194524_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194524_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194536_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194536_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194540_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194540_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194550_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194550_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194562_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194562_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:04:02.06 +42:01:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194591_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194591_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:18.55 +45:28:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.913 196927450274785792 089.32765314131 +45.48035392189 14.4964 13.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194593_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194593_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194602_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194602_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194603_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194603_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194611_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194611_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:02:40.11 +47:50:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.536 969752973479517568 090.66727522877 +47.84300158632 14.8894 14.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194612_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194612_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
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Considering the candidate 194643_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194643_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 194645_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194645_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:07:04.29 +43:37:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.866 961196230395290240 091.76798080454 +43.62192236236 14.7744 14.3135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194647_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194647_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:58:07.22 +44:56:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.493 196653667584324352 089.53066890331 +44.93909753755 14.7385 14.2784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194650_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194650_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:08:28.83 +46:28:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.160 963431674973670272 092.12007488321 +46.47836146643 14.9237 14.4001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194662_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194662_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:59.73 +44:02:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.921 197111927710804608 084.49902640194 +44.03515731599 14.7286 14.0299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194664_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194664_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194665_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194665_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
Preparing report for the candidate 194666_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194711_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 194711_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:02:02.72 +41:50:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.277 960759896078081536 090.51141856402 +41.84365110628 14.7475 14.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:57:23.92 +48:22:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146598_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 146598_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101942_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 101942_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188672_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 188672_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:59:44.12 +47:37:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69032_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 69032_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 05:37:57.09 +44:41:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-08_00-22-00_20.00sec_-4.90C_LIGHT_0026 did not pass the final checks
**** FOUND 06:14:58.99 +46:47:46.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 119s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:01:40.78 +43:38:48.0
05:58:04.10 +45:09:36.5
05:36:41.46 +43:17:59.3
06:14:00.35 +49:18:12.2
05:39:45.39 +44:56:08.6
05:36:58.52 +42:09:16.5
06:13:19.07 +41:52:44.2
05:40:17.80 +49:18:49.4
05:36:25.33 +42:06:51.4
06:25:09.90 +42:48:31.7
06:21:39.39 +42:45:08.7
05:48:33.25 +41:48:56.3
05:55:58.17 +46:42:37.8
06:12:10.13 +50:14:54.9
06:26:19.84 +41:59:10.0
06:09:44.74 +47:04:27.3
05:54:26.16 +41:58:44.9
06:03:22.99 +42:40:13.1
05:55:48.10 +42:30:30.2
06:23:09.77 +49:10:01.8
05:58:13.59 +42:51:14.2
05:39:19.03 +44:01:55.0
06:13:29.68 +41:58:07.9
06:02:31.99 +48:11:24.1
05:51:18.84 +43:17:46.2
05:56:33.85 +45:29:09.4
06:23:05.54 +49:11:44.3
05:37:19.36 +44:51:39.6
05:50:26.45 +44:11:29.2
06:00:04.44 +45:58:33.0
05:56:28.25 +47:43:41.9
05:48:38.67 +44:53:26.6
05:49:38.66 +47:49:49.4
05:50:28.68 +44:11:34.9
05:49:06.58 +47:17:58.1
05:54:37.54 +42:21:16.8
05:46:33.00 +45:16:05.8
05:41:02.56 +46:20:39.1
05:39:33.82 +49:48:34.9
06:01:46.35 +44:17:42.3
06:26:29.64 +49:54:11.4
05:48:18.83 +43:50:48.9
05:37:52.49 +43:02:32.5
05:56:58.19 +46:41:29.4
06:04:15.48 +46:54:36.1
06:09:10.38 +42:04:38.6
05:50:48.01 +47:35:37.0
06:18:39.33 +44:47:06.1
05:57:26.59 +46:34:08.9
05:58:27.40 +43:46:24.2
05:55:10.31 +48:15:51.2
05:54:26.84 +44:46:41.9
06:25:25.41 +43:24:39.5
05:53:58.30 +46:34:03.4
05:41:43.83 +42:01:00.9
05:46:41.02 +44:07:06.7
06:22:11.45 +44:11:23.6
06:13:49.90 +45:04:26.5
06:30:11.54 +46:26:04.7
########### Completed Aur-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:01:40.78 +43:38:48.0
05:58:04.10 +45:09:36.5
05:36:41.46 +43:17:59.3
06:14:00.35 +49:18:12.2
05:39:45.39 +44:56:08.6
05:36:58.52 +42:09:16.5
06:13:19.07 +41:52:44.2
05:40:17.80 +49:18:49.4
05:36:25.33 +42:06:51.4
06:25:09.90 +42:48:31.7
06:21:39.39 +42:45:08.7
05:48:33.25 +41:48:56.3
05:55:58.17 +46:42:37.8
06:12:10.13 +50:14:54.9
06:26:19.84 +41:59:10.0
06:09:44.74 +47:04:27.3
05:54:26.16 +41:58:44.9
06:03:22.99 +42:40:13.1
05:55:48.10 +42:30:30.2
06:23:09.77 +49:10:01.8
05:58:13.59 +42:51:14.2
05:39:19.03 +44:01:55.0
06:13:29.68 +41:58:07.9
06:02:31.99 +48:11:24.1
05:51:18.84 +43:17:46.2
05:56:33.85 +45:29:09.4
06:23:05.54 +49:11:44.3
05:37:19.36 +44:51:39.6
05:50:26.45 +44:11:29.2
06:00:04.44 +45:58:33.0
05:56:28.25 +47:43:41.9
05:48:38.67 +44:53:26.6
05:49:38.66 +47:49:49.4
05:50:28.68 +44:11:34.9
05:49:06.58 +47:17:58.1
05:54:37.54 +42:21:16.8
05:46:33.00 +45:16:05.8
05:41:02.56 +46:20:39.1
05:39:33.82 +49:48:34.9
06:01:46.35 +44:17:42.3
06:26:29.64 +49:54:11.4
05:48:18.83 +43:50:48.9
05:37:52.49 +43:02:32.5
05:56:58.19 +46:41:29.4
06:04:15.48 +46:54:36.1
06:09:10.38 +42:04:38.6
05:50:48.01 +47:35:37.0
06:18:39.33 +44:47:06.1
05:57:26.59 +46:34:08.9
05:58:27.40 +43:46:24.2
05:55:10.31 +48:15:51.2
05:54:26.84 +44:46:41.9
06:25:25.41 +43:24:39.5
05:53:58.30 +46:34:03.4
05:41:43.83 +42:01:00.9
05:46:41.02 +44:07:06.7
06:22:11.45 +44:11:23.6
06:13:49.90 +45:04:26.5
06:30:11.54 +46:26:04.7
###################################################################################
06:01:40.78 +43:38:48.0 -- not an asteroid (will add it to exclusion list)
05:58:04.10 +45:09:36.5 -- not an asteroid (will add it to exclusion list)
05:36:41.46 +43:17:59.3 -- not an asteroid (will add it to exclusion list)
06:14:00.35 +49:18:12.2 -- not an asteroid (will add it to exclusion list)
05:39:45.39 +44:56:08.6 -- not an asteroid (will add it to exclusion list)
05:36:58.52 +42:09:16.5 -- not an asteroid (will add it to exclusion list)
06:13:19.07 +41:52:44.2 -- not an asteroid (will add it to exclusion list)
05:40:17.80 +49:18:49.4 -- not an asteroid (will add it to exclusion list)
05:36:25.33 +42:06:51.4 -- not an asteroid (will add it to exclusion list)
06:25:09.90 +42:48:31.7 -- not an asteroid (will add it to exclusion list)
06:21:39.39 +42:45:08.7 -- not an asteroid (will add it to exclusion list)
05:48:33.25 +41:48:56.3 -- not an asteroid (will add it to exclusion list)
05:55:58.17 +46:42:37.8 -- not an asteroid (will add it to exclusion list)
06:12:10.13 +50:14:54.9 -- not an asteroid (will add it to exclusion list)
06:26:19.84 +41:59:10.0 -- not an asteroid (will add it to exclusion list)
06:09:44.74 +47:04:27.3 -- not an asteroid (will add it to exclusion list)
05:54:26.16 +41:58:44.9 -- not an asteroid (will add it to exclusion list)
06:03:22.99 +42:40:13.1 -- not an asteroid (will add it to exclusion list)
05:55:48.10 +42:30:30.2 -- not an asteroid (will add it to exclusion list)
06:23:09.77 +49:10:01.8 -- not an asteroid (will add it to exclusion list)
05:58:13.59 +42:51:14.2 -- not an asteroid (will add it to exclusion list)
05:39:19.03 +44:01:55.0 -- not an asteroid (will add it to exclusion list)
06:13:29.68 +41:58:07.9 -- not an asteroid (will add it to exclusion list)
06:02:31.99 +48:11:24.1 -- not an asteroid (will add it to exclusion list)
05:51:18.84 +43:17:46.2 -- not an asteroid (will add it to exclusion list)
05:56:33.85 +45:29:09.4 -- not an asteroid (will add it to exclusion list)
06:23:05.54 +49:11:44.3 -- not an asteroid (will add it to exclusion list)
05:37:19.36 +44:51:39.6 -- not an asteroid (will add it to exclusion list)
05:50:26.45 +44:11:29.2 -- not an asteroid (will add it to exclusion list)
06:00:04.44 +45:58:33.0 -- not an asteroid (will add it to exclusion list)
05:56:28.25 +47:43:41.9 -- not an asteroid (will add it to exclusion list)
05:48:38.67 +44:53:26.6 -- not an asteroid (will add it to exclusion list)
05:49:38.66 +47:49:49.4 -- not an asteroid (will add it to exclusion list)
05:50:28.68 +44:11:34.9 -- not an asteroid (will add it to exclusion list)
05:49:06.58 +47:17:58.1 -- not an asteroid (will add it to exclusion list)
05:54:37.54 +42:21:16.8 -- not an asteroid (will add it to exclusion list)
05:46:33.00 +45:16:05.8 -- not an asteroid (will add it to exclusion list)
05:41:02.56 +46:20:39.1 -- not an asteroid (will add it to exclusion list)
05:39:33.82 +49:48:34.9 -- not an asteroid (will add it to exclusion list)
06:01:46.35 +44:17:42.3 -- not an asteroid (will add it to exclusion list)
06:26:29.64 +49:54:11.4 -- not an asteroid (will add it to exclusion list)
05:48:18.83 +43:50:48.9 -- not an asteroid (will add it to exclusion list)
05:37:52.49 +43:02:32.5 -- not an asteroid (will add it to exclusion list)
05:56:58.19 +46:41:29.4 -- not an asteroid (will add it to exclusion list)
06:04:15.48 +46:54:36.1 -- not an asteroid (will add it to exclusion list)
06:09:10.38 +42:04:38.6 -- asteroid (will NOT add it to exclusion list)
05:50:48.01 +47:35:37.0 -- not an asteroid (will add it to exclusion list)
06:18:39.33 +44:47:06.1 -- not an asteroid (will add it to exclusion list)
05:57:26.59 +46:34:08.9 -- not an asteroid (will add it to exclusion list)
05:58:27.40 +43:46:24.2 -- not an asteroid (will add it to exclusion list)
05:55:10.31 +48:15:51.2 -- not an asteroid (will add it to exclusion list)
05:54:26.84 +44:46:41.9 -- not an asteroid (will add it to exclusion list)
06:25:25.41 +43:24:39.5 -- not an asteroid (will add it to exclusion list)
05:53:58.30 +46:34:03.4 -- not an asteroid (will add it to exclusion list)
05:41:43.83 +42:01:00.9 -- not an asteroid (will add it to exclusion list)
05:46:41.02 +44:07:06.7 -- not an asteroid (will add it to exclusion list)
06:22:11.45 +44:11:23.6 -- not an asteroid (will add it to exclusion list)
06:13:49.90 +45:04:26.5 -- not an asteroid (will add it to exclusion list)
06:30:11.54 +46:26:04.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:36:25.33 +42:06:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:41.46 +43:17:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:58.52 +42:09:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.36 +44:51:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.49 +43:02:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.03 +44:01:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:33.82 +49:48:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:45.39 +44:56:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:17.80 +49:18:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:02.56 +46:20:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:43.83 +42:01:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:33.00 +45:16:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:41.02 +44:07:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:18.83 +43:50:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:33.25 +41:48:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:38.67 +44:53:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.58 +47:17:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.66 +47:49:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:26.45 +44:11:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.68 +44:11:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:48.01 +47:35:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.84 +43:17:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:58.30 +46:34:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:26.16 +41:58:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:26.84 +44:46:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:37.54 +42:21:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.31 +48:15:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:48.10 +42:30:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:58.17 +46:42:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:28.25 +47:43:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.85 +45:29:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:58.19 +46:41:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:26.59 +46:34:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:04.10 +45:09:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:13.59 +42:51:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:27.40 +43:46:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:04.44 +45:58:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:40.78 +43:38:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:46.35 +44:17:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:31.99 +48:11:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:22.99 +42:40:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.48 +46:54:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:44.74 +47:04:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.13 +50:14:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:19.07 +41:52:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:29.68 +41:58:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:49.90 +45:04:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:00.35 +49:18:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:39.33 +44:47:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:39.39 +42:45:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:11.45 +44:11:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:05.54 +49:11:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:09.77 +49:10:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.90 +42:48:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:25.41 +43:24:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.84 +41:59:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.64 +49:54:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:11.54 +46:26:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
05:36:25.33 +42:06:51.4 -- not a known variable star
05:36:41.46 +43:17:59.3 -- not a known variable star
05:36:58.52 +42:09:16.5 -- a known variable star
05:37:19.36 +44:51:39.6 -- not a known variable star
05:37:52.49 +43:02:32.5 -- not a known variable star
05:39:19.03 +44:01:55.0 -- not a known variable star
05:39:33.82 +49:48:34.9 -- not a known variable star
05:39:45.39 +44:56:08.6 -- not a known variable star
05:40:17.80 +49:18:49.4 -- not a known variable star
05:41:02.56 +46:20:39.1 -- not a known variable star
05:41:43.83 +42:01:00.9 -- not a known variable star
05:46:33.00 +45:16:05.8 -- not a known variable star
05:46:41.02 +44:07:06.7 -- not a known variable star
05:48:18.83 +43:50:48.9 -- a known variable star
05:48:33.25 +41:48:56.3 -- not a known variable star
05:48:38.67 +44:53:26.6 -- not a known variable star
05:49:06.58 +47:17:58.1 -- not a known variable star
05:49:38.66 +47:49:49.4 -- not a known variable star
05:50:26.45 +44:11:29.2 -- a known variable star
05:50:28.68 +44:11:34.9 -- a known variable star
05:50:48.01 +47:35:37.0 -- a known variable star
05:51:18.84 +43:17:46.2 -- not a known variable star
05:53:58.30 +46:34:03.4 -- not a known variable star
05:54:26.16 +41:58:44.9 -- not a known variable star
05:54:26.84 +44:46:41.9 -- not a known variable star
05:54:37.54 +42:21:16.8 -- a known variable star
05:55:10.31 +48:15:51.2 -- not a known variable star
05:55:48.10 +42:30:30.2 -- not a known variable star
05:55:58.17 +46:42:37.8 -- not a known variable star
05:56:28.25 +47:43:41.9 -- not a known variable star
05:56:33.85 +45:29:09.4 -- not a known variable star
05:56:58.19 +46:41:29.4 -- not a known variable star
05:57:26.59 +46:34:08.9 -- not a known variable star
05:58:04.10 +45:09:36.5 -- not a known variable star
05:58:13.59 +42:51:14.2 -- not a known variable star
05:58:27.40 +43:46:24.2 -- not a known variable star
06:00:04.44 +45:58:33.0 -- not a known variable star
06:01:40.78 +43:38:48.0 -- not a known variable star
06:01:46.35 +44:17:42.3 -- not a known variable star
06:02:31.99 +48:11:24.1 -- not a known variable star
06:03:22.99 +42:40:13.1 -- not a known variable star
06:04:15.48 +46:54:36.1 -- not a known variable star
06:09:44.74 +47:04:27.3 -- a known variable star
06:12:10.13 +50:14:54.9 -- not a known variable star
06:13:19.07 +41:52:44.2 -- not a known variable star
06:13:29.68 +41:58:07.9 -- not a known variable star
06:13:49.90 +45:04:26.5 -- not a known variable star
06:14:00.35 +49:18:12.2 -- not a known variable star
06:18:39.33 +44:47:06.1 -- a known variable star
06:21:39.39 +42:45:08.7 -- not a known variable star
06:22:11.45 +44:11:23.6 -- not a known variable star
06:23:05.54 +49:11:44.3 -- not a known variable star
06:23:09.77 +49:10:01.8 -- not a known variable star
06:25:09.90 +42:48:31.7 -- not a known variable star
06:25:25.41 +43:24:39.5 -- not a known variable star
06:26:19.84 +41:59:10.0 -- not a known variable star
06:26:29.64 +49:54:11.4 -- not a known variable star
06:30:11.54 +46:26:04.7 -- not a known variable star
Found 50 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
58 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 58 (excluding asteroids and hot pixels, 50 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)2461138.72321875 -observatory V36
23:29:13.63 -05:42:21.8 Mercury (0.3mag)
02:31:07.64 +14:43:49.6 Venus (-3.9mag)
23:55:42.34 -01:34:22.4 Mars (1.2mag)
07:09:25.59 +22:51:20.3 Jupiter (-2.2mag)
00:25:41.00 +00:27:02.8 Saturn (0.9mag)
03:46:06.92 +19:42:22.3 Uranus (5.8mag)
00:09:48.30 -00:21:55.2 Neptune (7.8mag)
20:33:21.48 -22:52:27.3 Pluto (14.5mag)
17:46:43.89 -28:40:46.6 Moon (-10.9mag)
-rw-r--r-- 1 apache apache 362 Apr 8 00:25 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461138.72321875:
07:09:22.41 +22:51:23.9 Io (5.7mag)
07:09:15.31 +22:51:43.0 Europa (5.8mag)
07:09:45.95 +22:50:39.9 Ganymede (5.3mag)
07:08:50.55 +22:52:30.0 Callisto (6.5mag)
07:13:04.43 +22:42:46.8 Himalia (15.3mag)
07:09:22.96 +22:51:27.4 Thebe (16.2mag)
07:13:05.09 +23:11:58.1 Elara (17.3mag)
07:07:46.71 +23:35:24.8 Pasiphae (17.3mag)
07:17:55.07 +22:48:31.2 Carme (18.4mag)
00:25:43.88 +00:26:53.3 Titan (8.8mag)
00:25:46.07 +00:27:03.0 Rhea (10.1mag)
00:25:36.93 +00:28:21.6 Iapetus (11.5mag)
00:25:49.73 +00:26:48.3 Hyperion (14.8mag)
00:27:23.80 +00:36:39.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 00:25 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461138.72321875:
14:59:06.71 -10:09:19.2 JWST
13:41:45.51 +56:14:57.6 Chandra
08:04:45.85 -40:02:08.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 00:25 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461138.72321875 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:17.01 -28:20:33.8 13.9mag P/2010 H2 (Vales)
05:01:23.52 -70:02:36.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:54.87 +31:23:15.9 17.2mag C/2017 K2 (PANSTARRS)
17:30:55.19 +09:36:58.5 17.6mag C/2021 G2 (ATLAS)
23:07:59.49 +28:56:15.1 17.0mag C/2022 E2 (ATLAS)
04:20:17.19 +25:49:20.3 15.9mag C/2022 N2 (PANSTARRS)
09:02:05.42 +31:56:21.2 16.2mag C/2022 QE78 (ATLAS)
08:30:08.24 -01:00:07.4 17.3mag C/2022 R6 (PANSTARRS)
18:55:17.20 +17:52:13.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:59.19 -11:37:58.4 17.6mag P/2023 B1 (PANSTARRS)
09:11:38.51 -13:09:34.6 17.6mag C/2023 F3 (ATLAS)
21:45:51.34 +62:28:29.6 17.5mag C/2023 H5 (Lemmon)
19:25:07.89 -03:37:41.8 14.2mag C/2023 R1 (PANSTARRS)
21:41:51.69 +84:52:05.2 17.8mag C/2023 X2 (Lemmon)
06:15:00.45 +63:33:52.4 17.1mag C/2024 A1 (ATLAS)
04:55:53.37 +15:25:31.9 10.5mag C/2024 E1 (Wierzchos)
16:23:59.01 +05:06:43.0 17.4mag C/2024 G6 (ATLAS)
20:18:18.76 +13:12:25.4 14.7mag C/2024 J3 (ATLAS)
03:19:30.59 -23:35:48.2 16.4mag C/2024 T5 (ATLAS)
05:10:18.14 +47:17:16.5 17.7mag C/2025 J1 (Borisov)
14:10:58.05 +39:21:57.7 14.9mag C/2025 L1 (ATLAS)
03:13:21.04 -25:02:26.1 17.8mag C/2025 Q3 (ATLAS)
22:59:29.47 +19:48:35.3 9.8mag C/2025 R3 (PANSTARRS)
12:57:30.41 +02:31:28.4 17.5mag C/2025 Y1 (ATLAS)
02:04:07.96 +03:59:16.2 9.6mag C/2026 A1 (MAPS)
23:36:56.17 +35:41:04.3 14.3mag C/2026 B2 (Sun-Gao)
18:27:45.89 -10:07:14.5 12.3mag 10P/Tempel
15:10:27.48 +03:56:44.0 13.3mag 24P/Schaumasse
11:05:05.84 -01:47:25.6 15.7mag 29P/Schwassmann-Wachmann
17:57:52.35 -09:54:38.3 17.7mag 40P/Vaisala
10:38:26.90 -04:45:38.3 16.8mag 43P/Wolf-Harrington
01:36:40.33 +16:08:59.7 17.2mag 47P/Ashbrook-Jackson
06:56:48.79 +38:39:33.2 17.0mag 63P/Wild
23:18:59.50 -12:24:04.1 15.7mag 65P/Gunn
03:42:51.54 +18:29:30.2 15.9mag 76P/West-Kohoutek-Ikemura
00:48:29.81 +06:41:24.5 14.4mag 78P/Gehrels
22:38:59.51 -11:40:49.5 14.5mag 88P/Howell
01:48:42.90 +18:31:08.2 15.1mag 93P/Lovas
04:40:30.92 +31:51:00.7 16.3mag 123P/West-Hartley
08:19:52.56 +41:57:09.9 16.2mag 124P/Mrkos
02:21:17.62 +13:29:26.6 16.4mag 128P/Shoemaker-Holt
02:32:20.54 +13:31:04.6 17.5mag 131P/Mueller
00:46:03.23 +10:23:52.6 11.1mag 141P/Machholz
00:55:52.40 +01:57:18.1 11.1mag 141P-A/Machholz
23:45:15.71 -01:46:56.6 13.8mag 141P-D/Machholz
01:25:18.68 +03:39:04.0 17.9mag 141P-I/Machholz
00:40:45.69 -05:24:49.8 15.2mag 162P/SidingSpring
10:30:21.37 +31:22:55.1 17.9mag 164P/Christensen
06:22:08.97 +24:28:26.2 17.9mag 198P/ODAS
15:05:11.31 -00:56:36.9 17.4mag 210P/Christensen
21:15:23.65 -13:19:50.4 17.5mag 218P/LINEAR
17:13:41.40 -14:50:42.5 16.2mag 235P/LINEAR
05:17:54.11 +34:02:54.3 16.6mag 240P/NEAT
07:34:59.53 -06:02:41.4 17.6mag 242P/Spahr
15:45:21.29 +06:27:20.5 17.5mag 391P/Kowalski
07:31:30.41 +21:19:38.1 17.6mag 450P/LONEOS
05:24:44.32 +45:29:25.1 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 00:25 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 8 00:25 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 00:25 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
10:11:03.633 -05:31:15.36 AT 2026ics 2026-04-02.23 18.6573
11:09:42.183 +10:32:49.70 AT 2026icr 2026-03-24.33 20.476
10:16:29.552 -18:01:01.61 AT 2026icq 2026-03-25.18 20.2716
18:12:46.220 -18:40:42.30 AT 2026icp 2026-04-02.23 18.9
07:46:30.650 +27:23:24.16 AT 2026ico 2026-03-30.16 19.803
07:04:53.063 +10:28:54.71 AT 2026icn 2026-03-29.17 19.8144
10:09:06.230 +29:30:55.76 AT 2026icm 2026-03-27.16 20.1135
08:07:47.384 -00:23:25.65 AT 2026icl 2026-03-30.25 19.1418
07:33:52.396 +16:18:53.23 AT 2026ick 2026-03-30.19 19.5464
03:49:33.049 -49:30:53.67 AT 2026icj 2026-02-23.11 23.84
15:40:04.940 -18:30:53.00 AT 2026ici 2026-03-29.36 18.4
16:52:58.870 -62:16:14.10 AT 2026ich 2026-04-01.35 16.9
19:13:48.516 +60:10:55.03 AT 2026icg 2026-03-28.56 18.844
07:51:19.796 +21:17:20.06 AT 2026icf 2026-03-30.91 18.372
16:10:07.169 +56:12:02.29 AT 2026ice 2026-04-01.56 19.57
11:37:39.020 -44:29:30.90 AT 2026icd 2026-03-30.96 17.1
17:57:05.380 +48:58:47.80 AT 2026icc 2026-03-27.87 21.55
18:55:04.390 +55:02:09.27 AT 2026icb 2026-03-26.80 20.48
13:10:36.900 +47:58:12.10 AT 2026ica 2026-03-24.69 22.02
16:45:33.510 +54:24:32.89 AT 2026ibz 2026-03-30.82 20.28
-rw-r--r-- 1 apache apache 30K Apr 8 00:25 tns_transients_list.txt
