This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461143.8766,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.3766 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx1893924,2461143.8766,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx1893924 20260413.3766 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8766,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3766 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2786044,2461143.8766,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2786044 20260413.3766 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8766,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3766 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6037696455841949952,2461143.8766,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6037696455841949952 20260413.3766 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6028481929931396864,2461143.8766,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6028481929931396864 20260413.3766 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165955.59-294604.7,2461143.8766,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J165955.59-294604.7 20260413.3766 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165615.20-344327.8,2461143.8766,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J165615.20-344327.8 20260413.3766 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BZ Sco,2461143.8766,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BZ Sco 20260413.3766 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1558 Sco,2461143.8766,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1558 Sco 20260413.3766 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1162 Sco,2461143.8766,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1162 Sco 20260413.3766 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8766,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3766 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J163225.59-374813.2,2461143.8766,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J163225.59-374813.2 20260413.3766 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161626-3604.1,2461143.8766,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161626-3604.1 20260413.3766 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J164635.79-372157.7,2461143.8766,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J164635.79-372157.7 20260413.3766 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2956534,2461143.8766,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx2956534 20260413.3766 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J244.4015-34.9426,2461143.8766,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J244.4015-34.9426 20260413.3766 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170214.61-352748.7,2461143.8766,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170214.61-352748.7 20260413.3766 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3011143,2461143.8766,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3011143 20260413.3766 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.8766,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.3766 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165725.16-314730.0,2461143.8766,12.61,0.05,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
ASASSN-V J165725.16-314730.0 20260413.3766 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6026241022157031424,2461143.8766,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6026241022157031424 20260413.3766 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
First image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Last image: 2461143.87692016 13.04.2026 09:02:35.902 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.56
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): 5680
Objects passed selection criteria: 5673
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 4980.5
Average stars matched: 4840 (97.179 %)
Memory usage VmPeak: 112392 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 04:04:56 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
First image: 2461098.96724120 27.02.2026 11:12:39.640 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Last image: 2461143.87692016 13.04.2026 09:02:35.902 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 111
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
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: 24 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): 69295
Objects passed selection criteria: 69235
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 60981.2
Average stars matched: 58608.5 (96.109 %)
Memory usage VmPeak: 1924668 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 04:10:32 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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.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: 2461143.87624891
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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits exists and is non-empty
Saving wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits to local_wcs_cache/
'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits exists and is non-empty
Saving wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits to local_wcs_cache/
'wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits'
wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits exists and is non-empty
Saving wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits to local_wcs_cache/
'wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits' -> 'local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:56.510 -34:00:03.99
Angular distance between the image centers 0.0419 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 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:54.659 -34:00:01.69
Angular distance between the image centers 0.0355 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 16:41:56.510 -34:00:03.99
Second-epoch second image center 16:41:54.659 -34:00:01.69
Angular distance between the image centers 0.00643 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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits &> /tmp/tmp.gbOxM3UHnx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits &> /tmp/tmp.xwatnrM2Jv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits &> /tmp/tmp.DKFLerfltz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits &> /tmp/tmp.yzKxHDAm4I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
Found non-empty wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
The reference image (wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits) and catalog (wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat) found
'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat' -> 'wcsmag.cat'
Read 8448 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.2438 to 260.3527 deg, Dec -39.3236 to -28.2459 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 240.2438 to 260.3527 deg, Dec -39.3236 to -28.2459 deg
Loaded 13743 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): 6495 out of 6674 total matches.
Matched with Tycho-2 6674 out of 8448 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.631042
a=0.000000 b=1.000000 c=22.631042
From vast_summary.log: estimated ref. image limiting mag.: -8.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
2.4 pix Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
2.8 pix fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
2.8 pix fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Limiting magnitude estimates:
14.1 mag. Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
14.1 mag. Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
13.1 mag. fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
13.4 mag. fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.8 (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.gbOxM3UHnx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=8448
Got 8448 stars (including 7867 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 8448 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8269 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 955 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits -region wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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.xwatnrM2Jv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=572, passed=8450
Got 8450 stars (including 7869 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 8450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8242 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 956 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_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits -region wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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.DKFLerfltz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=298, passed=5315
Got 5315 stars (including 5012 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat
util/solve_plate_with_UCAC5 got 5315 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 253 to 310 (Dec -39.3 to -28.4)
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...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5247 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 5245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 957 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_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits -region wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.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.yzKxHDAm4I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=361, passed=5965
Got 5965 stars (including 5599 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 5965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 253 to 310 (Dec -39.3 to -28.4)
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...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 5847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 5848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.05"
Excluding outliers - 954 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits -region wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
Saving fully-calibrated image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits'
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits'
Preparing the HTML report for the field Sco-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20496.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 264s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20443_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20443_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:21:18.30 -34:19:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20451_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 20451_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20454_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20454_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:11:49.47 -36:35:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20481_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20481_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:34:20.34 -37:28:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20486_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20486_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:11:45.13 -37:02:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 1.279 5998435820504496128 242.93848379577 -37.04037599462 11.0413 10.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20495_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20495_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:13:10.99 -37:57:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 0.323 5997563151865273856 243.29569723393 -37.95231122193 11.0916 10.1917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20496_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 20496_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20499_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20499_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:11:35.55 -35:42:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 1.333 6022775640694349056 242.89856770772 -35.70047755915 11.0743 10.3004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20508_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 20508_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:09:00.71 -37:30:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 1.073 5998443036050567296 242.25326289661 -37.50077014147 11.2331 10.6786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01772_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 01772_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:03:32.18 -36:55:11.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 266s
Prepared the HTML report for the field Sco-03-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 ####
16:48:42.33 -29:48:17.6
16:12:24.26 -35:17:49.5
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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat to cache
SExtractor catalog cache: saved Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits exists and is non-empty
wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits exists and is non-empty
wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits exists and is non-empty
wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:56.510 -34:00:03.99
Angular distance between the image centers 0.0419 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 16:41:44.386 -34:00:08.14
Second-epoch image center 16:41:54.659 -34:00:01.69
Angular distance between the image centers 0.0355 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 16:41:56.510 -34:00:03.99
Second-epoch second image center 16:41:54.659 -34:00:01.69
Angular distance between the image centers 0.00643 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/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits &> /tmp/tmp.UnTmTzNYqT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits &> /tmp/tmp.1fWZO9Xhh5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits &> /tmp/tmp.60u4FgZN2S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits &> /tmp/tmp.xBMq10n2zq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
Found non-empty wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits and wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
The reference image (wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits) and catalog (wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat) found
'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat' -> 'wcsmag.cat'
Read 94880 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 240.1952 to 260.3527 deg, Dec -39.3356 to -28.2336 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 240.1952 to 260.3527 deg, Dec -39.3356 to -28.2336 deg
Loaded 13805 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): 9915 out of 11104 total matches.
Matched with Tycho-2 11104 out of 94880 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.379047
a=0.000000 b=1.000000 c=22.379047
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 76 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
2.2 pix Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
2.5 pix fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
2.4 pix fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Limiting magnitude estimates:
14.2 mag. Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
14.2 mag. Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
13.6 mag. fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
13.7 mag. fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.1 (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.UnTmTzNYqT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits' -> 'wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=5626, passed=94878
Got 94878 stars (including 89094 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat
util/solve_plate_with_UCAC5 got 94878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 93049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 93049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 93031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 957 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits -region wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.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.1fWZO9Xhh5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits' -> 'wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Checking if the catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat corresponding to the image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
WCS catalog name: wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=2, blended=5558, passed=95130
Got 95130 stars (including 89426 good ones) from the SExtractor catalog wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 95130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 92939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 92926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits -region wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.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.60u4FgZN2S (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2576, passed=52257
Got 52257 stars (including 49611 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat
util/solve_plate_with_UCAC5 got 52257 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 51619 with non-zero local correction accuracy
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 51620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 51620 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits -region wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.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.xBMq10n2zq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS-calibrated image found: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Checking if the catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat corresponding to the image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
WCS catalog name: wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3266, passed=59878
Got 59878 stars (including 56542 good ones) from the SExtractor catalog wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 59878 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 58712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 253 to 310 (Dec -39.3 to -28.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 58712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 58712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits -region wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.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_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_Sco-03-Q2b1x1_2026-02-27_05-12-39_20.00sec_-15.00C_LIGHT_0014.fits
Saving fully-calibrated image wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_Sco-03-Q2b1x1_2026-02-27_05-13-22_20.00sec_-15.00C_LIGHT_0015.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-01-37_20.00sec_-4.90C_LIGHT_0485.fits
Saving fully-calibrated image wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Sco-03-Q2b1x1_040320_TTUQ2b1x1_18714_1pSkD51G/wcs_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486.fits
Preparing the HTML report for the field Sco-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out113014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73121.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 362s
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: 15s
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Considering the candidate 113014_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113014_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113016_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113016_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113019_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113019_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113031_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113031_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113038_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113038_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113040_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113040_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
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Considering the candidate 113047_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113047_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:17:23.27 -30:52:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113048_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113048_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:02:37.82 -31:58:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:48:42.34 -29:48:17.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 113158_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113158_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 113213_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113213_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 113298_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113298_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 113388_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113388_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:31:20.79 -34:43:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 113408_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113408_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:55:03.29 -36:21:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113425_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113425_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:50:22.45 -37:42:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113435_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113435_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:35:27.16 -32:09:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113482_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113482_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:12:14.42 -37:00:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113484_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113484_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:26:49.15 -31:14:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113486_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113486_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:57:18.69 -33:15:30.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 113491_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113491_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:24:01.06 -33:17:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113495_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113495_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:24:29.14 -37:18:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113525_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113525_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:30:27.92 -35:15:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113546_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113546_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:15:04.65 -31:04:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113571_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113571_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:33:57.82 -32:09:09.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113604_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113604_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:40:52.45 -30:02:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113609_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113609_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:36:48.29 -36:24:38.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113630_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113630_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:03:23.25 -35:02:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113641_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113641_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:33:54.81 -30:39:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113664_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113664_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:32:27.54 -36:22:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113690_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113690_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113703_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113703_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:59:34.29 -32:59:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113705_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113705_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:00:57.48 -37:31:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113711_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113711_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113712_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113712_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113748_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113748_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:21:13.73 -36:49:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113753_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113753_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:03:26.87 -36:52:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113761_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113761_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:56:43.21 -37:53:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113767_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113767_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:38:02.91 -36:54:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113778_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113778_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:02:37.79 -35:20:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113779_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113779_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113780_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113780_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:56:14.18 -35:02:35.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113790_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113790_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113794_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113794_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:38:39.32 -30:59:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113797_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113797_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113801_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113801_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:46:11.47 -31:15:18.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113817_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113817_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:51:51.84 -37:58:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113820_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113820_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:31:32.53 -34:52:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113822_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113822_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113832_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113832_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:16:22.13 -31:36:48.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113837_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113837_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113842_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113842_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113850_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113850_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113852_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113852_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113853_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113853_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:59:14.22 -35:54:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113854_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113854_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113862_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113862_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113867_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113867_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113870_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 113870_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113880_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 113880_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:36:45.71 -33:31:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69388_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 69388_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:00:27.64 -30:39:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85329_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 85329_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:46:17.90 -31:02:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86834_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 86834_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:46:27.83 -31:16:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32479_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 32479_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:14:36.39 -34:06:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86799_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 86799_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:57:58.86 -31:18:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76059_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 76059_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:23:17.98 -32:40:10.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106272_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 106272_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:57:51.03 -31:22:06.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31561_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 31561_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:21:18.32 -34:19:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14258_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 14258_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:03:32.16 -36:55:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105510_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 105510_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:16:10.89 -33:24:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 73121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36744_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
Preparing report for the candidate 36744_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 77121_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:46:02.47 -29:43:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87946_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 87946_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:54:29.25 -31:26:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33702_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 33702_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:09:37.36 -33:53:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110609_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 110609_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 16:39:40.16 -33:01:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17937_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486
The candidate 17937_fd_Sco-03-Q2b1x1_2026-04-13_04-02-35_20.00sec_-4.90C_LIGHT_0486 did not pass the final checks
**** FOUND 17:00:04.61 -36:25:51.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 378s
Prepared the HTML report for the field Sco-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:48:42.33 -29:48:17.6
16:12:24.26 -35:17:49.5
16:48:53.74 -35:56:57.4
16:59:41.34 -34:29:58.3
16:32:16.14 -35:31:18.8
16:24:53.91 -30:40:25.8
17:00:55.20 -30:59:27.4
16:59:56.03 -29:46:03.1
16:56:15.27 -34:43:29.9
16:30:11.34 -36:15:07.3
16:22:43.65 -36:23:58.4
16:46:01.13 -36:33:06.6
16:28:09.04 -38:06:47.3
16:32:25.53 -37:48:13.6
16:16:25.57 -36:04:07.7
16:46:35.73 -37:21:57.4
16:39:16.50 -31:26:26.4
16:17:36.47 -34:56:35.9
17:02:14.43 -35:27:50.4
16:34:01.17 -34:31:32.8
16:25:17.58 -33:10:33.8
16:52:48.97 -34:06:04.6
16:57:24.95 -31:47:34.8
########### Completed Sco-03-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 ####
16:48:42.33 -29:48:17.6
16:12:24.26 -35:17:49.5
16:48:53.74 -35:56:57.4
16:59:41.34 -34:29:58.3
16:32:16.14 -35:31:18.8
16:24:53.91 -30:40:25.8
17:00:55.20 -30:59:27.4
16:59:56.03 -29:46:03.1
16:56:15.27 -34:43:29.9
16:30:11.34 -36:15:07.3
16:22:43.65 -36:23:58.4
16:46:01.13 -36:33:06.6
16:28:09.04 -38:06:47.3
16:32:25.53 -37:48:13.6
16:16:25.57 -36:04:07.7
16:46:35.73 -37:21:57.4
16:39:16.50 -31:26:26.4
16:17:36.47 -34:56:35.9
17:02:14.43 -35:27:50.4
16:34:01.17 -34:31:32.8
16:25:17.58 -33:10:33.8
16:57:24.95 -31:47:34.8
16:52:48.97 -34:06:04.6
###################################################################################
16:48:42.33 -29:48:17.6 -- asteroid (will NOT add it to exclusion list)
16:12:24.26 -35:17:49.5 -- not an asteroid (will add it to exclusion list)
16:48:53.74 -35:56:57.4 -- not an asteroid (will add it to exclusion list)
16:59:41.34 -34:29:58.3 -- not an asteroid (will add it to exclusion list)
16:32:16.14 -35:31:18.8 -- not an asteroid (will add it to exclusion list)
16:24:53.91 -30:40:25.8 -- not an asteroid (will add it to exclusion list)
17:00:55.20 -30:59:27.4 -- not an asteroid (will add it to exclusion list)
16:59:56.03 -29:46:03.1 -- not an asteroid (will add it to exclusion list)
16:56:15.27 -34:43:29.9 -- not an asteroid (will add it to exclusion list)
16:30:11.34 -36:15:07.3 -- asteroid (will NOT add it to exclusion list)
16:22:43.65 -36:23:58.4 -- not an asteroid (will add it to exclusion list)
16:46:01.13 -36:33:06.6 -- not an asteroid (will add it to exclusion list)
16:28:09.04 -38:06:47.3 -- not an asteroid (will add it to exclusion list)
16:32:25.53 -37:48:13.6 -- not an asteroid (will add it to exclusion list)
16:16:25.57 -36:04:07.7 -- not an asteroid (will add it to exclusion list)
16:46:35.73 -37:21:57.4 -- not an asteroid (will add it to exclusion list)
16:39:16.50 -31:26:26.4 -- not an asteroid (will add it to exclusion list)
16:17:36.47 -34:56:35.9 -- not an asteroid (will add it to exclusion list)
17:02:14.43 -35:27:50.4 -- not an asteroid (will add it to exclusion list)
16:34:01.17 -34:31:32.8 -- not an asteroid (will add it to exclusion list)
16:25:17.58 -33:10:33.8 -- not an asteroid (will add it to exclusion list)
16:57:24.95 -31:47:34.8 -- not an asteroid (will add it to exclusion list)
16:52:48.97 -34:06:04.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:12:24.26 -35:17:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
16:16:25.57 -36:04:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
16:17:36.47 -34:56:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:22:43.65 -36:23:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:24:53.91 -30:40:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:25:17.58 -33:10:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:28:09.04 -38:06:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:16.14 -35:31:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:32:25.53 -37:48:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:34:01.17 -34:31:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:39:16.50 -31:26:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:01.13 -36:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:35.73 -37:21:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:48:53.74 -35:56:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
16:52:48.97 -34:06:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:56:15.27 -34:43:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
16:57:24.95 -31:47:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:41.34 -34:29:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
16:59:56.03 -29:46:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:00:55.20 -30:59:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:14.43 -35:27:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
16:12:24.26 -35:17:49.5 -- not a known variable star
16:16:25.57 -36:04:07.7 -- a known variable star
16:17:36.47 -34:56:35.9 -- not a known variable star
16:22:43.65 -36:23:58.4 -- a known variable star
16:24:53.91 -30:40:25.8 -- not a known variable star
16:25:17.58 -33:10:33.8 -- not a known variable star
16:28:09.04 -38:06:47.3 -- not a known variable star
16:32:16.14 -35:31:18.8 -- not a known variable star
16:32:25.53 -37:48:13.6 -- a known variable star
16:34:01.17 -34:31:32.8 -- not a known variable star
16:39:16.50 -31:26:26.4 -- not a known variable star
16:46:01.13 -36:33:06.6 -- a known variable star
16:46:35.73 -37:21:57.4 -- a known variable star
16:48:53.74 -35:56:57.4 -- not a known variable star
16:52:48.97 -34:06:04.6 -- a known variable star
16:56:15.27 -34:43:29.9 -- a known variable star
16:57:24.95 -31:47:34.8 -- a known variable star
16:59:41.34 -34:29:58.3 -- not a known variable star
16:59:56.03 -29:46:03.1 -- a known variable star
17:00:55.20 -30:59:27.4 -- not a known variable star
17:02:14.43 -35:27:50.4 -- a known variable star
Found 11 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 ####
16:12:24.26 -35:17:49.5
16:16:25.57 -36:04:07.7
16:17:36.47 -34:56:35.9
16:22:43.65 -36:23:58.4
16:24:53.91 -30:40:25.8
16:25:17.58 -33:10:33.8
16:28:09.04 -38:06:47.3
16:32:16.14 -35:31:18.8
16:32:25.53 -37:48:13.6
16:34:01.17 -34:31:32.8
16:39:16.50 -31:26:26.4
16:46:01.13 -36:33:06.6
16:46:35.73 -37:21:57.4
16:48:53.74 -35:56:57.4
16:52:48.97 -34:06:04.6
16:56:15.27 -34:43:29.9
16:57:24.95 -31:47:34.8
16:59:41.34 -34:29:58.3
16:59:56.03 -29:46:03.1
17:00:55.20 -30:59:27.4
17:02:14.43 -35:27:50.4
16:11:45.13 -37:02:25.5
16:13:10.99 -37:57:08.5
16:11:35.55 -35:42:01.4
16:09:00.71 -37:30:03.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461143.87624891 -observatory V36
23:53:45.27 -03:26:14.2 Mercury (0.1mag)
02:55:52.52 +16:50:56.7 Venus (-3.9mag)
00:10:23.34 +00:02:37.9 Mars (1.2mag)
07:11:28.44 +22:48:06.1 Jupiter (-2.1mag)
00:28:00.56 +00:41:39.4 Saturn (0.9mag)
03:47:09.03 +19:45:43.1 Uranus (5.8mag)
00:10:29.73 -00:17:32.9 Neptune (7.8mag)
20:33:38.04 -22:52:30.1 Pluto (14.5mag)
22:11:25.43 -12:43:36.1 Moon (-9.4mag)
-rw-r--r-- 1 apache apache 361 Apr 13 04:04 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461143.87624891:
07:11:29.75 +22:48:00.6 Io (5.8mag)
07:11:40.72 +22:47:39.3 Europa (5.9mag)
07:11:23.38 +22:48:23.4 Ganymede (5.3mag)
07:11:46.78 +22:47:37.5 Callisto (6.6mag)
07:14:55.44 +22:36:58.0 Himalia (15.3mag)
07:11:28.14 +22:48:04.2 Thebe (16.2mag)
07:15:03.37 +23:06:55.8 Elara (17.3mag)
07:10:10.63 +23:29:28.7 Pasiphae (17.4mag)
07:19:51.61 +22:45:51.5 Carme (18.5mag)
00:28:10.77 +00:41:49.8 Titan (8.8mag)
00:28:06.24 +00:41:44.5 Rhea (10.1mag)
00:27:45.41 +00:42:13.8 Iapetus (11.5mag)
00:28:15.11 +00:41:43.4 Hyperion (14.8mag)
00:29:39.52 +00:50:44.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 13 04:05 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461143.87624891:
15:25:28.75 -14:23:05.1 JWST
10:10:29.70 +42:54:56.3 Chandra
19:07:07.00 -09:46:09.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 13 04:04 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461143.87624891 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:50:52.72 -28:37:38.4 13.9mag P/2010 H2 (Vales)
05:04:52.44 -69:47:13.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:53.59 +31:25:11.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:39.98 +10:14:09.5 17.6mag C/2021 G2 (ATLAS)
23:09:30.75 +29:07:35.2 17.0mag C/2022 E2 (ATLAS)
04:26:11.37 +25:57:59.8 16.0mag C/2022 N2 (PANSTARRS)
09:02:53.22 +31:59:56.6 16.2mag C/2022 QE78 (ATLAS)
08:30:41.60 -00:25:59.5 17.3mag C/2022 R6 (PANSTARRS)
18:54:19.65 +18:18:41.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:41:30.31 -11:33:35.8 17.5mag P/2023 B1 (PANSTARRS)
09:08:53.17 -12:18:22.2 17.6mag C/2023 F3 (ATLAS)
21:51:32.01 +62:45:18.2 17.5mag C/2023 H5 (Lemmon)
19:21:23.58 -03:41:29.9 14.2mag C/2023 R1 (PANSTARRS)
21:37:05.96 +85:33:02.3 17.8mag C/2023 X2 (Lemmon)
06:16:44.45 +63:31:32.9 17.1mag C/2024 A1 (ATLAS)
05:07:35.16 +17:24:29.6 10.9mag C/2024 E1 (Wierzchos)
16:20:56.20 +05:57:36.4 17.4mag C/2024 G6 (ATLAS)
20:20:02.91 +14:33:57.0 14.6mag C/2024 J3 (ATLAS)
03:24:01.44 -22:47:13.9 16.4mag C/2024 T5 (ATLAS)
05:14:30.18 +45:56:52.3 17.7mag C/2025 J1 (Borisov)
13:49:44.15 +43:40:43.2 15.1mag C/2025 L1 (ATLAS)
03:21:09.80 -25:48:21.3 17.8mag C/2025 Q3 (ATLAS)
23:23:25.99 +19:18:32.7 8.9mag C/2025 R3 (PANSTARRS)
12:55:15.36 +02:51:06.8 17.4mag C/2025 Y1 (ATLAS)
03:04:43.00 +02:56:34.0 12.4mag C/2026 A1 (MAPS)
23:52:05.40 +36:43:39.0 14.5mag C/2026 B2 (Sun-Gao)
18:37:49.49 -09:51:32.2 12.0mag 10P/Tempel
15:03:49.56 +03:28:33.3 13.8mag 24P/Schaumasse
11:03:31.28 -01:36:42.7 15.7mag 29P/Schwassmann-Wachmann
18:00:07.68 -09:42:29.6 17.9mag 40P/Vaisala
10:37:43.11 -04:18:40.4 16.9mag 43P/Wolf-Harrington
01:44:36.98 +17:02:21.9 17.2mag 47P/Ashbrook-Jackson
07:05:57.17 +37:34:26.2 17.0mag 63P/Wild
23:25:42.05 -11:46:02.6 15.7mag 65P/Gunn
03:56:16.37 +20:20:42.7 15.9mag 76P/West-Kohoutek-Ikemura
00:59:47.10 +07:42:43.8 14.4mag 78P/Gehrels
22:55:01.34 -10:10:00.4 14.6mag 88P/Howell
02:03:00.24 +19:56:18.6 15.1mag 93P/Lovas
04:49:53.34 +32:08:44.2 16.2mag 123P/West-Hartley
08:25:19.48 +39:34:16.7 16.2mag 124P/Mrkos
02:29:10.17 +14:04:34.8 16.4mag 128P/Shoemaker-Holt
02:42:23.75 +14:10:15.2 17.5mag 131P/Mueller
01:12:26.53 +12:19:02.6 10.8mag 141P/Machholz
01:21:43.38 +03:53:17.8 10.8mag 141P-A/Machholz
00:08:18.62 -00:06:02.4 13.1mag 141P-D/Machholz
01:51:48.75 +05:38:12.4 17.8mag 141P-I/Machholz
00:55:04.15 -02:50:39.4 15.1mag 162P/SidingSpring
10:29:13.03 +31:01:07.6 18.0mag 164P/Christensen
06:31:40.23 +24:19:30.3 18.0mag 198P/ODAS
14:56:05.63 -00:20:43.4 17.6mag 210P/Christensen
21:31:10.76 -12:04:55.9 17.6mag 218P/LINEAR
17:15:49.52 -14:14:50.5 16.1mag 235P/LINEAR
05:28:49.94 +34:29:40.2 16.7mag 240P/NEAT
07:37:13.79 -05:27:15.2 17.7mag 242P/Spahr
22:10:21.28 -21:40:15.4 18.0mag 260P/McNaught
15:43:38.34 +06:48:56.3 17.5mag 391P/Kowalski
07:33:12.75 +21:21:23.6 17.6mag 450P/LONEOS
05:32:03.58 +45:11:09.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 13 04:04 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:35.90 ASASSN-26co 2026-04-7.15 14.93
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
-rw-r--r-- 1 apache apache 5.8K Apr 13 04:04 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
-rw-r--r-- 1 apache apache 188K Apr 13 04:04 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:15:51.420 +01:05:21.68 AT 2026isr 2026-03-23.82 22.65
10:13:53.630 +05:15:26.71 AT 2026isq 2026-03-23.63 22.63
13:46:10.060 +01:20:22.93 AT 2026isp 2026-03-08.91 20.81
10:37:05.160 -01:41:10.54 AT 2026iso 2026-02-05.76 20.81
14:04:58.698 +08:42:54.25 AT 2026isn 2026-04-07.34 19.61
17:07:59.639 +03:14:36.58 AT 2026ism 2026-04-07.44 19.9709
12:35:03.843 +16:11:04.99 AT 2026isl 2026-04-07.25 20.1748
12:18:45.074 +08:22:57.24 AT 2026isk 2026-04-07.25 19.4891
18:56:30.261 +78:17:13.39 AT 2026isj 2026-03-27.43 20.1324
19:03:47.920 +77:35:41.47 AT 2026isi 2026-04-07.45 19.3393
12:30:44.663 -02:08:00.62 AT 2026ish 2026-03-28.50 19.51
13:14:05.683 -16:32:12.44 AT 2026isg 2026-04-07.51 19.32
19:24:27.622 +59:09:12.86 AT 2026isf 2026-03-22.52 20.4885
16:04:49.647 +18:09:53.48 AT 2026ise 2026-04-05.40 19.9772
10:37:43.207 -02:42:01.74 AT 2026isd 2026-03-25.48 20.07
16:35:34.990 +26:38:38.36 AT 2026isc 2026-04-07.19 19.39
09:57:36.948 -43:21:35.60 AT 2026isb 2026-04-05.43 19.8
12:08:58.779 -20:41:57.54 AT 2026isa 2026-04-06.51 19.6
15:44:09.789 -09:40:35.89 AT 2026irz 2026-04-02.40 19.2513
15:39:54.203 +04:05:53.02 AT 2026iry 2026-04-07.34 19.8481
-rw-r--r-- 1 apache apache 30K Apr 13 04:04 tns_transients_list.txt
