This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh
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
ATO J233.3458-27.1604,2461143.9098,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J233.3458-27.1604 20260413.4098 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J150448.15-251349.7,2461143.9098,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J150448.15-251349.7 20260413.4098 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J152515.31-293026.4,2461143.9098,12.08,0.05,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 J152515.31-293026.4 20260413.4098 12.08CV 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 J150133-2949.7,2461143.9098,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J150133-2949.7 20260413.4098 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AI Lib,2461143.9098,13.08,0.05,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
AI Lib 20260413.4098 13.08CV 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 J150152-2520.8,2461143.9098,11.44,0.05,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 J150152-2520.8 20260413.4098 11.44CV 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
SSS_J152157.0-301727,2461143.9098,11.85,0.05,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
SSS_J152157.0-301727 20260413.4098 11.85CV 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 J151150-2154.8,2461143.9098,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J151150-2154.8 20260413.4098 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J152008-2732.1,2461143.9098,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J152008-2732.1 20260413.4098 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J153749.08-293306.9,2461143.9098,12.45,0.05,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 J153749.08-293306.9 20260413.4098 12.45CV 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 J151050-2741.4,2461143.9098,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J151050-2741.4 20260413.4098 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J150952.14-260118.1,2461143.9098,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J150952.14-260118.1 20260413.4098 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.87662444 19.03.2026 09:02:10.352 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
First image: 2461118.87662444 19.03.2026 09:02:10.352 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Last image: 2461143.91011065 13.04.2026 09:50:23.560 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.33
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): 7266
Objects passed selection criteria: 7243
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 5306
Average stars matched: 4664.25 (87.9052 %)
Memory usage VmPeak: 112124 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 05:05:36 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.87662444 19.03.2026 09:02:10.352 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
First image: 2461118.87662444 19.03.2026 09:02:10.352 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Last image: 2461143.91011065 13.04.2026 09:50:23.560 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.02
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: 19 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): 45772
Objects passed selection criteria: 45691
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 34258.8
Average stars matched: 30266.5 (88.3468 %)
Memory usage VmPeak: 143240 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 05:06:49 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/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
SExtractor catalog cache: saved Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat to cache
SExtractor catalog cache: saved Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.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/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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: 2461143.90948258
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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits exists and is non-empty
Saving wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits to local_wcs_cache/
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits' -> 'local_wcs_cache/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits'
wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits exists and is non-empty
Saving wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits to local_wcs_cache/
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits' -> 'local_wcs_cache/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits'
wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits exists and is non-empty
Saving wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits to local_wcs_cache/
'wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits' -> 'local_wcs_cache/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits'
wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits exists and is non-empty
Saving wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits to local_wcs_cache/
'wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits' -> 'local_wcs_cache/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:21:54.615 -26:00:54.11
Second-epoch image center 15:21:36.868 -26:01:58.15
Angular distance between the image centers 0.0688 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 15:21:54.615 -26:00:54.11
Second-epoch image center 15:21:37.125 -26:01:34.95
Angular distance between the image centers 0.0665 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 15:21:36.868 -26:01:58.15
Second-epoch second image center 15:21:37.125 -26:01:34.95
Angular distance between the image centers 0.00652 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/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits &> /tmp/tmp.BBGSfxRBVb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits &> /tmp/tmp.Dix7ZBMyV4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits &> /tmp/tmp.2zjMegM2pq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits &> /tmp/tmp.0cyRjqTQQW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
Found non-empty wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
The reference image (wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits) and catalog (wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat) found
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat' -> 'wcsmag.cat'
Read 7634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.3411 to 239.4609 deg, Dec -31.2938 to -20.5007 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 221.3411 to 239.4609 deg, Dec -31.2938 to -20.5007 deg
Loaded 7368 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): 5295 out of 5414 total matches.
Matched with Tycho-2 5414 out of 7634 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.766542
a=0.000000 b=1.000000 c=22.766542
From vast_summary.log: estimated ref. image limiting mag.: -8.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.7 pix Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
2.5 pix Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
3.6 pix fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
3.6 pix fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Limiting magnitude estimates:
14.4 mag. Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
14.5 mag. Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
13.8 mag. fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
13.7 mag. fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.3 (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.BBGSfxRBVb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits' -> 'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS-calibrated image found: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Checking if the catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS catalog name: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=7634
Got 7634 stars (including 7211 good ones) from the SExtractor catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 7634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
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: 966 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 293 to 349 (Dec -31.3 to -20.5)
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: 966 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 7517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits -region wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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.Dix7ZBMyV4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits' -> 'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS-calibrated image found: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Checking if the catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS catalog name: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=470, passed=7479
Got 7479 stars (including 7003 good ones) from the SExtractor catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 7479 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7348 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 7347 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits -region wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.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.2zjMegM2pq (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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS_IMAGE_NAME=wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS-calibrated image found: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Checking if the catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS catalog name: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=419, passed=6057
Got 6057 stars (including 5636 good ones) from the SExtractor catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat
util/solve_plate_with_UCAC5 got 6057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
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: 962 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
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 293 to 349 (Dec -31.3 to -20.5)
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: 962 matched stars entering correct_measured_positions(), 5884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 962 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_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits -region wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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.0cyRjqTQQW (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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS_IMAGE_NAME=wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS-calibrated image found: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Checking if the catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS catalog name: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=384, passed=5538
Got 5538 stars (including 5151 good ones) from the SExtractor catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat
util/solve_plate_with_UCAC5 got 5538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
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: 963 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
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 293 to 349 (Dec -31.3 to -20.5)
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: 963 matched stars entering correct_measured_positions(), 5359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits -region wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits'
Saving fully-calibrated image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits'
Saving fully-calibrated image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits'
Saving fully-calibrated image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits'
Preparing the HTML report for the field Lib-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22345.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20940_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 20940_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:01:46.66 -30:14:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21649_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 21649_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:20:08.28 -27:32:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 2.004 6213999095203086208 230.03430210735 -27.53580601761 9.9311 8.4690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21958_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 21958_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:40:08.39 -21:41:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 0.069 6241300827914370304 235.03496737614 -21.68667728148 11.6172 11.0450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22199_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22199_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:32:38.90 -22:08:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 0.585 6251739316434009600 233.16215780403 -22.14382511376 11.5034 10.6401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22275_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22275_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:41:23.47 -22:57:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.58, MAG_FAINT_SEARCH_LIMIT=12.56)GAIADR2_OUTPUT=# 0.264 6240148848967827200 235.34771650556 -22.95194091301 11.7332 11.1390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22307_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22307_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:37:42.33 -21:52:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.465 6241211453936766080 234.42651053560 -21.87888706200 11.7556 11.0100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22333_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22333_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:35:06.74 -21:42:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.325 6241250147301583488 233.77817480968 -21.71416393071 11.8606 11.2584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22336_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22336_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:41:11.65 -22:59:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.472 6240147199700380160 235.29841094995 -22.99077397432 11.8169 11.2199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22341_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22341_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:31:56.07 -22:05:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 4.786 6251755018834506496 232.98275881114 -22.08296814492 12.0360 11.4209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22345_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22345_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:40:49.21 -22:38:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 0.597 6240924794938445568 235.20490542112 -22.64591964280 11.7116 10.8882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22385_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 22385_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:40:45.19 -29:53:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06272_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 06272_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:24:19.76 -22:54:44.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lib-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
SExtractor catalog cache: saved Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat to cache
SExtractor catalog cache: saved Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Creating symlink local_wcs_cache/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits exists and is non-empty
wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits exists and is non-empty
wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits exists and is non-empty
wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:21:54.615 -26:00:54.11
Second-epoch image center 15:21:36.868 -26:01:58.15
Angular distance between the image centers 0.0688 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 15:21:54.615 -26:00:54.11
Second-epoch image center 15:21:37.125 -26:01:34.95
Angular distance between the image centers 0.0665 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 15:21:36.868 -26:01:58.15
Second-epoch second image center 15:21:37.125 -26:01:34.95
Angular distance between the image centers 0.00652 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/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits &> /tmp/tmp.dpIJlehEq7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits &> /tmp/tmp.9mkuLhr3Fb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits &> /tmp/tmp.XsaS0zbovt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits &> /tmp/tmp.0gCaETbuod
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
Found non-empty wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits and wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
The reference image (wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits) and catalog (wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat) found
'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat' -> 'wcsmag.cat'
Read 51045 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 221.3037 to 239.4934 deg, Dec -31.3007 to -20.4574 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 221.3037 to 239.4934 deg, Dec -31.3007 to -20.4574 deg
Loaded 7432 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): 5767 out of 6291 total matches.
Matched with Tycho-2 6291 out of 51045 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.577823
a=0.000000 b=1.000000 c=22.577823
From vast_summary.log: estimated ref. image limiting mag.: -8.02
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
2.3 pix Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
3.5 pix fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
3.5 pix fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Limiting magnitude estimates:
14.6 mag. Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
14.6 mag. Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
13.9 mag. fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
13.8 mag. fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dpIJlehEq7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits' -> 'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS_IMAGE_NAME=wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS-calibrated image found: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Checking if the catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits alredy exist and is non-empty...
Catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
WCS catalog name: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2624, passed=51038
Got 51038 stars (including 48352 good ones) from the SExtractor catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat
util/solve_plate_with_UCAC5 got 51038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 965 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(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 50168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 50166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 50166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 965 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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits -region wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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.9mkuLhr3Fb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits' -> 'wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS_IMAGE_NAME=wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS-calibrated image found: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Checking if the catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits alredy exist and is non-empty...
Catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat corresponding to the image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
WCS catalog name: wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2801, passed=54385
Got 54385 stars (including 51521 good ones) from the SExtractor catalog wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat
util/solve_plate_with_UCAC5 got 54385 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 53318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 53318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 53318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits -region wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.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.XsaS0zbovt (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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS_IMAGE_NAME=wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS-calibrated image found: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Checking if the catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
WCS catalog name: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2718, passed=33057
Got 33057 stars (including 30312 good ones) from the SExtractor catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat
util/solve_plate_with_UCAC5 got 33057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
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: 963 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 31955 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 293 to 349 (Dec -31.3 to -20.5)
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: 963 matched stars entering correct_measured_positions(), 31955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 31956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits -region wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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.0gCaETbuod (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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS_IMAGE_NAME=wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS-calibrated image found: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Checking if the catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat corresponding to the image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
WCS catalog name: wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2621, passed=31079
Got 31079 stars (including 28434 good ones) from the SExtractor catalog wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat
util/solve_plate_with_UCAC5 got 31079 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 965 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(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 30066 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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 30063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 30063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 965 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_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits -region wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-10_20.00sec_-14.90C_LIGHT_0126.fits
Saving fully-calibrated image wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_Lib-05-Q2b1x1_2026-03-19_04-02-56_20.00sec_-15.00C_LIGHT_0127.fits
Saving fully-calibrated image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-49-29_20.00sec_-5.00C_LIGHT_0535.fits
Saving fully-calibrated image wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.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_Lib-05-Q2b1x1_045238_TTUQ2b1x1_22530_0bBe5wdh/wcs_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536.fits
Preparing the HTML report for the field Lib-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out12744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72400.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 8s
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Considering the candidate 66053_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 66053_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:02:45.07 -29:35:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.653 6212003687758402304 225.68771609859 -29.58732166205 12.1601 11.6901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66054_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 66054_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 67538_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 67538_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 67902_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 67902_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 69110_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 69110_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 69445_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 69445_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:24:10.52 -22:53:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70506_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 70506_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:16:14.75 -22:24:23.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70797_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 70797_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 71064_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 71064_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:13:53.57 -26:09:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 71216_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 71216_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:13:35.03 -25:18:06.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 71524_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 71524_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:08:56.69 -26:28:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71812_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 71812_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:31:07.31 -23:38:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71970_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 71970_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 72400_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 72400_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 72413_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 72413_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:09:44.44 -23:58:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72664_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 72664_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:24:22.53 -25:46:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73256_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 73256_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:29:25.94 -28:51:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73675_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 73675_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:37:42.16 -26:38:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73816_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 73816_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:29:06.12 -24:28:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74007_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 74007_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:34:22.66 -25:03:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75026_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 75026_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:27:43.41 -25:09:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75513_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 75513_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 75752_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 75752_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 30765_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 30765_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 08867_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 08867_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 11148_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 11148_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:41:15.37 -29:02:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06346_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 06346_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 64875_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 64875_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 29945_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 29945_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 04970_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 04970_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 07987_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 07987_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:10:15.44 -29:34:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37914_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 37914_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 19150_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 19150_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 08646_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 08646_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 18020_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 18020_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 12744_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 12744_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
**** FOUND 15:08:36.45 -28:40:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.892 6212468265782029952 227.15104383636 -28.67572982355 11.9325 10.4489 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 27067_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
Preparing report for the candidate 27067_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
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Considering the candidate 42673_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536
The candidate 42673_fd_Lib-05-Q2b1x1_2026-04-13_04-50-23_20.00sec_-5.00C_LIGHT_0536 did not pass the final checks
