This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP
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
OY Cep,2461132.9277,9.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OY Cep 20260402.4277 9.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2286710682257185152,2461132.9277,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2286710682257185152 20260402.4277 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2285277331412357632,2461132.9277,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2285277331412357632 20260402.4277 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 2284328628971984896,2461132.9277,12.30,0.05,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
Gaia DR3 2284328628971984896 20260402.4277 12.30CV 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 2284233796094719744,2461132.9277,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2284233796094719744 20260402.4277 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2284415451734640128,2461132.9277,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2284415451734640128 20260402.4277 12.21CV 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
Gaia DR3 2286707525457593472,2461132.9277,12.31,0.05,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
Gaia DR3 2286707525457593472 20260402.4277 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
Gaia DR3 2285183636701260928,2461132.9277,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2285183636701260928 20260402.4277 12.11CV 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 2286717730300082816,2461132.9277,12.10,0.05,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
Gaia DR3 2286717730300082816 20260402.4277 12.10CV 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 2284419407401013248,2461132.9277,12.16,0.05,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 2284419407401013248 20260402.4277 12.16CV 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 2285168999452550016,2461132.9277,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2285168999452550016 20260402.4277 11.83CV 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
Gaia DR3 2286710927071682176,2461132.9277,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2286710927071682176 20260402.4277 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2286726320234449024,2461132.9277,11.12,0.05,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 2286726320234449024 20260402.4277 11.12CV 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
Gaia DR3 2284437721141515904,2461132.9277,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2284437721141515904 20260402.4277 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0392 Dra,2461132.9277,13.12,0.05,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
V0392 Dra 20260402.4277 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
NSVS J2125044+764630,2461132.9277,12.52,0.05,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
NSVS J2125044+764630 20260402.4277 12.52CV 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
V1054 Cep,2461132.9277,13.04,0.05,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
V1054 Cep 20260402.4277 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
AM Cep,2461132.9277,11.31,0.05,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
AM Cep 20260402.4277 11.31CV 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
NSVS J2139594+755506,2461132.9277,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2139594+755506 20260402.4277 11.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
NSVS J2108226+754207,2461132.9277,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2108226+754207 20260402.4277 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2134422+755948,2461132.9277,11.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2134422+755948 20260402.4277 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.95775807 19.03.2026 10:59:00.297 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461118.95775807 19.03.2026 10:59:00.297 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461132.92794174 02.04.2026 10:16:04.166 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 3 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): 10004
Objects passed selection criteria: 9974
Measurements per detected object (mean, median, min, max): 3.0 3.5 2 4
Measurements per selected object (mean, median, min, max): 3.0 4.0 2 4
Average stars detected per image: 7864.25
Average stars matched: 7648 (97.2502 %)
Memory usage VmPeak: 115744 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:18:09 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: 2461118.95775807 19.03.2026 10:59:00.297 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461118.95775807 19.03.2026 10:59:00.297 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461132.92794174 02.04.2026 10:16:04.166 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 13 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): 62424
Objects passed selection criteria: 62270
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 46498.5
Average stars matched: 44893.5 (96.5483 %)
Memory usage VmPeak: 164272 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:19:09 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/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
SExtractor catalog cache: saved Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.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/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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: 2461132.92743369
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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
Saving wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits to local_wcs_cache/
'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits'
wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits exists and is non-empty
Saving wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits'
wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits'
wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits'
The image scale is 5.87"/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 20:00:00.947 +77:30:25.41
Second-epoch image center 19:59:54.599 +77:30:28.11
Angular distance between the image centers 0.01 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 20:00:00.947 +77:30:25.41
Second-epoch image center 19:59:54.682 +77:30:20.11
Angular distance between the image centers 0.01 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 19:59:54.599 +77:30:28.11
Second-epoch second image center 19:59:54.682 +77:30:20.11
Angular distance between the image centers 0.00222 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/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.rPK4sjeuAF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits &> /tmp/tmp.aBpBWYDku4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits &> /tmp/tmp.OnpdOS6hOe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits &> /tmp/tmp.j20DnPsnuh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat' -> 'wcsmag.cat'
Read 12067 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 252.4096 to 346.4619 deg, Dec +70.4651 to +82.7909 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 252.4096 to 346.4619 deg, Dec 70.4651 to 82.7909 deg
Loaded 14571 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): 6915 out of 7265 total matches.
Matched with Tycho-2 7265 out of 12067 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.869160
a=0.000000 b=1.000000 c=22.869160
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
2.4 pix Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
3.7 pix fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
3.7 pix fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Limiting magnitude estimates:
15.2 mag. Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
15.1 mag. Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
14.1 mag. fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
14.1 mag. fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.5 (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.rPK4sjeuAF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=797, passed=12067
Got 12067 stars (including 11253 good ones) from the SExtractor catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 12067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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.aBpBWYDku4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits' -> 'wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Checking if the catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS catalog name: wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=12084
Got 12084 stars (including 11268 good ones) from the SExtractor catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 12084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 802 to 865 (Dec 70.5 to 82.8)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits -region wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.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.OnpdOS6hOe (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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=527, passed=6037
Got 6037 stars (including 5507 good ones) from the SExtractor catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 6037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (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 0.010410 (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 803 to 865 (Dec 70.7 to 82.7)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 803 to 865 (Dec 70.7 to 82.7)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits -region wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.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.j20DnPsnuh (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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=542, passed=6075
Got 6075 stars (including 5531 good ones) from the SExtractor catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 6075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (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 0.010410 (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 803 to 865 (Dec 70.7 to 82.7)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 803 to 865 (Dec 70.7 to 82.7)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits -region wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits'
Saving fully-calibrated image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits'
Saving fully-calibrated image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits'
Preparing the HTML report for the field Dra-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out05110.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20557_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 20557_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 22:17:34.02 +79:46:41.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 07381_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 07381_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 21:20:02.73 +77:50:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05110_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 05110_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 08861_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 08861_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 20:11:26.07 +80:10:35.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Dra-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 ####
21:09:39.04 +75:53:15.4
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/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
SExtractor catalog cache: saved Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits exists and is non-empty
wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits exists and is non-empty
The image scale is 5.87"/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 20:00:00.947 +77:30:25.41
Second-epoch image center 19:59:54.599 +77:30:28.11
Angular distance between the image centers 0.01 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 20:00:00.947 +77:30:25.41
Second-epoch image center 19:59:54.682 +77:30:20.11
Angular distance between the image centers 0.01 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 19:59:54.599 +77:30:28.11
Second-epoch second image center 19:59:54.682 +77:30:20.11
Angular distance between the image centers 0.00222 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/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.MaaiqKNdIl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits &> /tmp/tmp.d6077FScEx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits &> /tmp/tmp.mG8u2Px01o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits &> /tmp/tmp.qxszYJzDds
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat' -> 'wcsmag.cat'
Read 74965 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 252.0295 to 346.5832 deg, Dec +70.4215 to +82.7934 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 252.0295 to 346.5832 deg, Dec 70.4215 to 82.7934 deg
Loaded 14717 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): 6431 out of 7491 total matches.
Matched with Tycho-2 7491 out of 74965 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.711257
a=0.000000 b=1.000000 c=22.711257
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 47 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
2.1 pix Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
3.4 pix fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
3.4 pix fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Limiting magnitude estimates:
15.4 mag. Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
15.3 mag. Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
14.1 mag. fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
14.1 mag. fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
All-image limiting magnitude estimate: 14.1 (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.MaaiqKNdIl (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=5016, passed=74949
Got 74949 stars (including 69842 good ones) from the SExtractor catalog wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 74949 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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.d6077FScEx (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits' -> 'wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Checking if the catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat corresponding to the image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
WCS catalog name: wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=5096, passed=74368
Got 74368 stars (including 69181 good ones) from the SExtractor catalog wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 74368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 802 to 865 (Dec 70.4 to 82.8)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits -region wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.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.mG8u2Px01o (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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2516, passed=28666
Got 28666 stars (including 26126 good ones) from the SExtractor catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 28666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (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 0.010410 (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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.73"
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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits -region wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.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.qxszYJzDds (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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2588, passed=28828
Got 28828 stars (including 26220 good ones) from the SExtractor catalog wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 28828 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (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 0.010410 (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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
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 803 to 865 (Dec 70.6 to 82.8)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.74"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits -region wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_Dra-02-Q2b1x1_2026-03-19_05-59-00_20.00sec_-14.90C_LIGHT_0201.fits
Saving fully-calibrated image wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_Dra-02-Q2b1x1_2026-03-19_06-00-11_20.00sec_-14.90C_LIGHT_0202.fits
Saving fully-calibrated image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-15-20_20.00sec_-15.00C_LIGHT_0086.fits
Saving fully-calibrated image wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.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_2026-04-02_CI_Dra-02-Q2b1x1_051645_TTUQ2b1x1_2660_GB66WuzP/wcs_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087.fits
Preparing the HTML report for the field Dra-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out90112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out90955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out29884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90177.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 10s
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Considering the candidate 90112_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90112_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 20:16:16.47 +75:24:52.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 90130_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90130_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90131_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90131_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 21:47:47.52 +78:15:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.922 2284259497178627968 326.94733131774 +78.26193927096 12.1116 11.5420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90132_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90132_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 22:04:41.43 +79:07:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.581 2284405526066508160 331.17340320804 +79.12078894535 11.8531 11.3138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90134_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90134_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90138_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90138_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90145_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90145_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 22:10:01.83 +79:31:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.018 2285193081332901248 332.51376205604 +79.53211485470 11.8091 11.2982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90146_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90146_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90147_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90147_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90148_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90148_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90150_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90150_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90159_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90159_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90160_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90160_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90165_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90165_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 21:35:31.41 +75:30:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 5.804 2283329653938255872 323.88731018652 +75.50111283097 11.2182 10.6414 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90166_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90166_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 22:08:00.50 +78:51:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 5.722 2284389342629793152 331.99648766243 +78.85202528910 11.2211 10.6869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90168_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90168_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90169_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90169_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90176_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90176_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90177_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 90177_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 90678_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90678_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 17:48:33.12 +79:19:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90751_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90751_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 20:05:22.37 +73:26:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90844_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90844_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 18:28:14.98 +73:45:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90848_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90848_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 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 90856_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90856_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 18:19:30.51 +76:35:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90891_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90891_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 18:29:22.05 +77:33:51.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 90903_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90903_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:05:47.37 +80:30:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90917_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90917_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 18:32:57.41 +74:38:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90955_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 90955_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:06:41.91 +80:57:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.287 2295128891173200000 286.67964929431 +80.96270756166 13.5861 12.9363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91114_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91114_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:26:45.57 +73:21:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91118_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91118_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:20:29.18 +78:08:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.085 2293069059217174784 290.11930499258 +78.14592088362 13.4811 13.0456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91133_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91133_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:09:54.50 +74:37:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91136_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91136_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 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 91161_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91161_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 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 91194_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91194_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 19:33:19.21 +76:27:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91213_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91213_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 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 91214_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 91214_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 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 74932_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 74932_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 40599_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 40599_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 30850_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 30850_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 21:09:38.95 +75:53:15.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 67973_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 67973_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 40853_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 40853_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 37448_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 37448_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 66684_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 66684_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 20:11:26.04 +80:10:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29884_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 29884_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 36870_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
Preparing report for the candidate 36870_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
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Considering the candidate 52922_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 52922_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 21:20:02.60 +77:50:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12352_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087
The candidate 12352_fd_Dra-02-Q2b1x1_2026-04-02_05-16-04_20.00sec_-15.00C_LIGHT_0087 did not pass the final checks
**** FOUND 18:35:45.90 +73:25:27.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 41s
Prepared the HTML report for the field Dra-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
21:09:39.04 +75:53:15.4
21:08:21.65 +75:42:08.0
21:34:40.24 +75:59:48.4
21:39:56.01 +75:55:10.3
21:25:02.73 +76:46:27.9
21:41:24.44 +76:23:14.3
21:45:17.43 +78:33:23.9
17:59:45.87 +77:41:44.0
22:17:58.70 +80:01:29.4
22:11:29.36 +80:15:12.1
22:06:42.63 +78:33:09.2
22:05:00.93 +78:26:55.9
22:07:35.55 +79:19:46.0
22:16:41.23 +79:54:14.9
22:04:50.72 +79:33:03.2
22:22:39.64 +80:09:44.0
22:13:30.13 +79:12:27.1
22:02:46.93 +79:22:23.1
22:18:49.33 +80:04:08.4
22:14:33.19 +80:09:18.8
22:09:16.57 +79:18:48.1
########### Completed Dra-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 ####
21:09:39.04 +75:53:15.4
22:17:58.70 +80:01:29.4
22:11:29.36 +80:15:12.1
22:06:42.63 +78:33:09.2
22:05:00.93 +78:26:55.9
22:07:35.55 +79:19:46.0
22:16:41.23 +79:54:14.9
22:04:50.72 +79:33:03.2
22:22:39.64 +80:09:44.0
22:13:30.13 +79:12:27.1
22:02:46.93 +79:22:23.1
22:18:49.33 +80:04:08.4
22:14:33.19 +80:09:18.8
22:09:16.57 +79:18:48.1
17:59:45.87 +77:41:44.0
21:25:02.73 +76:46:27.9
21:45:17.43 +78:33:23.9
21:41:24.44 +76:23:14.3
21:39:56.01 +75:55:10.3
21:08:21.65 +75:42:08.0
21:34:40.24 +75:59:48.4
###################################################################################
21:09:39.04 +75:53:15.4 -- not an asteroid (will add it to exclusion list)
22:17:58.70 +80:01:29.4 -- not an asteroid (will add it to exclusion list)
22:11:29.36 +80:15:12.1 -- not an asteroid (will add it to exclusion list)
22:06:42.63 +78:33:09.2 -- not an asteroid (will add it to exclusion list)
22:05:00.93 +78:26:55.9 -- not an asteroid (will add it to exclusion list)
22:07:35.55 +79:19:46.0 -- not an asteroid (will add it to exclusion list)
22:16:41.23 +79:54:14.9 -- not an asteroid (will add it to exclusion list)
22:04:50.72 +79:33:03.2 -- not an asteroid (will add it to exclusion list)
22:22:39.64 +80:09:44.0 -- not an asteroid (will add it to exclusion list)
22:13:30.13 +79:12:27.1 -- not an asteroid (will add it to exclusion list)
22:02:46.93 +79:22:23.1 -- not an asteroid (will add it to exclusion list)
22:18:49.33 +80:04:08.4 -- not an asteroid (will add it to exclusion list)
22:14:33.19 +80:09:18.8 -- not an asteroid (will add it to exclusion list)
22:09:16.57 +79:18:48.1 -- not an asteroid (will add it to exclusion list)
17:59:45.87 +77:41:44.0 -- not an asteroid (will add it to exclusion list)
21:25:02.73 +76:46:27.9 -- not an asteroid (will add it to exclusion list)
21:45:17.43 +78:33:23.9 -- not an asteroid (will add it to exclusion list)
21:41:24.44 +76:23:14.3 -- not an asteroid (will add it to exclusion list)
21:39:56.01 +75:55:10.3 -- not an asteroid (will add it to exclusion list)
21:08:21.65 +75:42:08.0 -- not an asteroid (will add it to exclusion list)
21:34:40.24 +75:59:48.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:59:45.87 +77:41:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:08:21.65 +75:42:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:39.04 +75:53:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:25:02.73 +76:46:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:34:40.24 +75:59:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:39:56.01 +75:55:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:41:24.44 +76:23:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:45:17.43 +78:33:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:02:46.93 +79:22:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:04:50.72 +79:33:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:05:00.93 +78:26:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:06:42.63 +78:33:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
22:07:35.55 +79:19:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
22:09:16.57 +79:18:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:11:29.36 +80:15:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:13:30.13 +79:12:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
22:14:33.19 +80:09:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
22:16:41.23 +79:54:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
22:17:58.70 +80:01:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:18:49.33 +80:04:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
22:22:39.64 +80:09:44.0 -- 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)
17:59:45.87 +77:41:44.0 -- a known variable star
21:08:21.65 +75:42:08.0 -- a known variable star
21:09:39.04 +75:53:15.4 -- a known variable star
21:25:02.73 +76:46:27.9 -- a known variable star
21:34:40.24 +75:59:48.4 -- a known variable star
21:39:56.01 +75:55:10.3 -- a known variable star
21:41:24.44 +76:23:14.3 -- a known variable star
21:45:17.43 +78:33:23.9 -- a known variable star
22:02:46.93 +79:22:23.1 -- not a known variable star
22:04:50.72 +79:33:03.2 -- not a known variable star
22:05:00.93 +78:26:55.9 -- not a known variable star
22:06:42.63 +78:33:09.2 -- not a known variable star
22:07:35.55 +79:19:46.0 -- not a known variable star
22:09:16.57 +79:18:48.1 -- not a known variable star
22:11:29.36 +80:15:12.1 -- not a known variable star
22:13:30.13 +79:12:27.1 -- not a known variable star
22:14:33.19 +80:09:18.8 -- not a known variable star
22:16:41.23 +79:54:14.9 -- not a known variable star
22:17:58.70 +80:01:29.4 -- not a known variable star
22:18:49.33 +80:04:08.4 -- not a known variable star
22:22:39.64 +80:09:44.0 -- not a known variable star
Found 13 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
21 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:59:45.87 +77:41:44.0
21:08:21.65 +75:42:08.0
21:09:39.04 +75:53:15.4
21:25:02.73 +76:46:27.9
21:34:40.24 +75:59:48.4
21:39:56.01 +75:55:10.3
21:41:24.44 +76:23:14.3
21:45:17.43 +78:33:23.9
22:02:46.93 +79:22:23.1
22:04:50.72 +79:33:03.2
22:05:00.93 +78:26:55.9
22:06:42.63 +78:33:09.2
22:07:35.55 +79:19:46.0
22:09:16.57 +79:18:48.1
22:11:29.36 +80:15:12.1
22:13:30.13 +79:12:27.1
22:14:33.19 +80:09:18.8
22:16:41.23 +79:54:14.9
22:17:58.70 +80:01:29.4
22:18:49.33 +80:04:08.4
22:22:39.64 +80:09:44.0
20:16:16.47 +75:24:52.8
21:47:47.52 +78:15:42.2
22:04:41.43 +79:07:14.6
22:10:01.83 +79:31:55.8
21:35:31.41 +75:30:03.8
22:08:00.50 +78:51:03.1
19:06:41.91 +80:57:47.4
19:20:29.18 +78:08:47.9
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.92743369 -observatory V36
23:05:35.89 -07:28:07.0 Mercury (0.4mag)
02:03:48.35 +12:09:29.3 Venus (-3.9mag)
23:39:07.47 -03:23:25.9 Mars (1.2mag)
07:07:29.51 +22:54:14.7 Jupiter (-2.2mag)
00:23:02.65 +00:10:19.7 Saturn (0.9mag)
03:45:01.07 +19:38:47.0 Uranus (5.8mag)
00:09:00.86 -00:26:57.6 Neptune (7.8mag)
20:32:59.43 -22:52:37.9 Pluto (14.5mag)
12:52:26.79 -09:53:46.2 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 05:18 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.92743369:
07:07:37.31 +22:53:58.7 Io (5.7mag)
07:07:42.23 +22:53:49.7 Europa (5.8mag)
07:07:38.31 +22:53:50.3 Ganymede (5.3mag)
07:07:45.34 +22:53:34.9 Callisto (6.5mag)
07:11:19.18 +22:48:46.4 Himalia (15.3mag)
07:07:33.63 +22:54:05.6 Thebe (16.1mag)
07:11:11.29 +23:16:35.7 Elara (17.2mag)
07:05:27.06 +23:41:21.6 Pasiphae (17.3mag)
07:16:05.46 +22:50:41.1 Carme (18.4mag)
00:22:55.17 +00:10:44.5 Titan (8.8mag)
00:23:00.62 +00:10:26.6 Rhea (10.1mag)
00:23:11.80 +00:12:14.9 Iapetus (11.5mag)
00:22:53.12 +00:10:27.6 Hyperion (14.8mag)
00:24:49.43 +00:20:30.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 05:18 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.92743369:
14:22:24.18 -04:40:22.9 JWST
19:58:06.73 +01:44:37.9 Chandra
08:48:57.59 -49:44:24.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 05:18 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.92743369 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:47.22 -28:02:37.6 14.0mag P/2010 H2 (Vales)
04:57:46.16 -70:20:43.9 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.71 +31:21:19.2 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.84 +08:54:45.0 17.6mag C/2021 G2 (ATLAS)
23:06:06.73 +28:44:51.5 17.0mag C/2022 E2 (ATLAS)
04:13:47.78 +25:39:19.9 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.98 +31:49:55.2 16.1mag C/2022 QE78 (ATLAS)
08:29:48.66 -01:40:07.9 17.3mag C/2022 R6 (PANSTARRS)
18:56:02.17 +17:22:05.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.28 -11:42:35.0 17.6mag P/2023 B1 (PANSTARRS)
09:15:12.67 -14:08:54.8 17.5mag C/2023 F3 (ATLAS)
21:38:51.50 +62:11:25.4 17.4mag C/2023 H5 (Lemmon)
19:28:30.67 -03:34:42.6 14.3mag C/2023 R1 (PANSTARRS)
21:42:55.27 +84:09:16.8 17.8mag C/2023 X2 (Lemmon)
06:13:58.04 +63:37:25.6 17.0mag C/2024 A1 (ATLAS)
04:41:45.35 +12:47:31.5 10.1mag C/2024 E1 (Wierzchos)
16:27:02.98 +04:09:38.3 17.4mag C/2024 G6 (ATLAS)
20:16:01.39 +11:43:56.5 14.8mag C/2024 J3 (ATLAS)
03:14:35.69 -24:32:14.7 16.4mag C/2024 T5 (ATLAS)
05:05:50.66 +48:52:35.9 17.6mag C/2025 J1 (Borisov)
14:33:35.13 +33:20:43.5 14.7mag C/2025 L1 (ATLAS)
03:04:59.33 -24:13:18.7 17.7mag C/2025 Q3 (ATLAS)
22:45:42.70 +19:45:25.0 10.7mag C/2025 R3 (PANSTARRS)
13:00:00.78 +02:08:36.9 17.5mag C/2025 Y1 (ATLAS)
01:20:18.41 +02:43:54.8 8.3mag C/2026 A1 (MAPS)
23:19:13.62 +34:22:49.1 14.1mag C/2026 B2 (Sun-Gao)
18:16:25.25 -10:23:22.7 12.6mag 10P/Tempel
15:17:05.33 +04:23:41.5 12.8mag 24P/Schaumasse
11:07:05.47 -02:00:12.4 15.7mag 29P/Schwassmann-Wachmann
17:54:22.85 -10:08:51.6 17.6mag 40P/Vaisala
10:39:54.27 -05:18:29.7 16.6mag 43P/Wolf-Harrington
01:27:47.63 +15:08:10.2 17.1mag 47P/Ashbrook-Jackson
06:47:04.75 +39:51:11.8 17.1mag 63P/Wild
23:11:17.08 -13:07:50.9 15.7mag 65P/Gunn
03:28:14.20 +16:18:30.8 15.8mag 76P/West-Kohoutek-Ikemura
00:35:56.85 +05:31:58.9 14.5mag 78P/Gehrels
22:20:25.87 -13:21:13.6 14.5mag 88P/Howell
01:33:02.27 +16:52:24.5 15.1mag 93P/Lovas
04:30:26.43 +31:29:43.0 16.3mag 123P/West-Hartley
08:14:40.12 +44:37:28.6 16.2mag 124P/Mrkos
02:12:33.96 +12:49:12.8 16.4mag 128P/Shoemaker-Holt
02:21:07.50 +12:45:17.0 17.4mag 131P/Mueller
00:17:25.18 +08:07:04.6 11.6mag 141P/Machholz
00:27:35.56 -00:10:43.4 11.6mag 141P-A/Machholz
23:20:26.01 -03:34:17.3 14.5mag 141P-D/Machholz
00:56:02.97 +01:24:50.3 18.0mag 141P-I/Machholz
00:24:44.26 -08:15:39.6 15.3mag 162P/SidingSpring
10:32:22.82 +31:42:20.5 17.7mag 164P/Christensen
06:11:35.90 +24:36:00.0 17.8mag 198P/ODAS
15:15:01.65 -01:40:53.9 17.2mag 210P/Christensen
20:56:31.17 -14:43:26.1 17.3mag 218P/LINEAR
17:10:13.79 -15:28:55.2 16.2mag 235P/LINEAR
05:05:54.55 +33:28:29.0 16.5mag 240P/NEAT
07:32:52.52 -06:44:53.5 17.6mag 242P/Spahr
15:46:52.47 +06:01:58.4 17.6mag 391P/Kowalski
07:29:57.21 +21:16:36.0 17.6mag 450P/LONEOS
05:16:47.61 +45:50:14.5 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 05:18 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
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
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
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
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 2 05:18 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:03:36.117 -67:58:13.34 SN 2026hkg 2026-03-27.12 18.505
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
-rw-r--r-- 1 apache apache 29K Apr 2 05:18 tns_transients_list.txt
