This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI
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!
TCP 2026 04 13.4667* 00 10 42.47 +54 03 38.9 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.9667,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.4667 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 33 59.03 +54 05 13.1 12.3 U Cas 9 0
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 J003358.96+540513.3,2461143.9667,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J003358.96+540513.3 20260413.4667 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 09 14.45 +55 08 32.2 11.8 U Cas 9 0
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
NSVS 1559961,2461143.9667,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1559961 20260413.4667 11.79CV 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!
TCP 2026 04 13.4667* 00 18 33.39 +53 39 14.3 11.9 U Cas 9 0
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 J001833.41+533914.7,2461143.9667,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J001833.41+533914.7 20260413.4667 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 16 09.98 +55 24 24.2 12.1 U Cas 9 0
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 J001609.91+552423.8,2461143.9667,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J001609.91+552423.8 20260413.4667 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 12 01.36 +55 13 32.3 11.9 U Cas 9 0
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 J001201.35+551332.4,2461143.9667,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J001201.35+551332.4 20260413.4667 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 08 53.35 +55 48 16.7 12.8 U Cas 9 0
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 J000853.28+554816.7,2461143.9667,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J000853.28+554816.7 20260413.4667 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 06 42.73 +52 27 32.4 12.2 U Cas 9 0
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
V0856 Cas,2461143.9667,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
V0856 Cas 20260413.4667 12.23CV 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!
TCP 2026 04 13.4667* 00 21 10.91 +53 59 23.4 11.9 U Cas 9 0
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
NSVS J0021110+535925,2461143.9667,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0021110+535925 20260413.4667 11.91CV 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!
TCP 2026 04 13.4667* 00 27 55.07 +57 38 36.8 12.8 U Cas 9 0
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 J002755.08+573835.9,2461143.9667,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J002755.08+573835.9 20260413.4667 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 14 03.07 +55 52 37.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.9667,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.4667 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 19 18.95 +55 23 57.5 12.6 U Cas 9 0
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 J001918.67+552358.2,2461143.9667,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J001918.67+552358.2 20260413.4667 12.58CV 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!
TCP 2026 04 13.4667* 00 25 19.47 +54 00 14.1 11.3 U Cas 9 0
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 J002519.56+540015.2,2461143.9667,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J002519.56+540015.2 20260413.4667 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 23 51 03.48 +51 41 45.8 12.5 U Cas 9 0
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
NSVS J2351036+514143,2461143.9667,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2351036+514143 20260413.4667 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 03 22.64 +57 44 53.2 12.8 U Cas 9 0
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
EY Cas,2461143.9667,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
EY Cas 20260413.4667 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4667* 00 11 13.20 +52 32 31.6 11.0 U Cas 9 0
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 J001113.26+523231.6,2461143.9667,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J001113.26+523231.6 20260413.4667 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.58312155 27.12.2025 01:59:31.702 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461036.58312155 27.12.2025 01:59:31.702 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461143.96710016 13.04.2026 11:12:27.454 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 27923
Objects passed selection criteria: 27728
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 17625.2
Average stars matched: 17155.8 (97.3362 %)
Memory usage VmPeak: 131480 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 06:16:09 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.58312155 27.12.2025 01:59:31.702 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
First image: 2461036.58312155 27.12.2025 01:59:31.702 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Last image: 2461143.96710016 13.04.2026 11:12:27.454 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 140
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 52 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): 185358
Objects passed selection criteria: 184876
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 126930
Average stars matched: 121958 (96.0829 %)
Memory usage VmPeak: 2009896 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 06:20:56 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
SExtractor catalog cache: saved Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.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/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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: 2461143.96635750
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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits'
wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
Saving wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits to local_wcs_cache/
'wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits' -> 'local_wcs_cache/wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits'
wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits'
wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits exists and is non-empty
Saving wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits to local_wcs_cache/
'wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits' -> 'local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.845 +53:59:35.63
Second-epoch image center 23:59:31.229 +53:58:21.05
Angular distance between the image centers 0.0778 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 00:00:01.845 +53:59:35.63
Second-epoch image center 23:59:33.992 +53:58:24.31
Angular distance between the image centers 0.0711 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 23:59:31.229 +53:58:21.05
Second-epoch second image center 23:59:33.992 +53:58:24.31
Angular distance between the image centers 0.00683 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/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.eyAJbu1z88
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.iIfWG2uMZc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits &> /tmp/tmp.4Fr8T20Kpv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits &> /tmp/tmp.4WXlAxesbP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
Found non-empty wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
The reference image (wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat) found
'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat' -> 'wcsmag.cat'
Read 30002 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0009 to 359.9993 deg, Dec +47.6490 to +59.3704 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 0.0009 to 359.9993 deg, Dec 47.6490 to 59.3704 deg
Loaded 163379 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): 15843 out of 17844 total matches.
Matched with Tycho-2 17844 out of 30002 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958037
a=0.000000 b=1.000000 c=22.958037
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.00
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.00
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
2.5 pix Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
2.3 pix fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
2.5 pix fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Limiting magnitude estimates:
15.0 mag. Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
15.0 mag. Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
13.0 mag. fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
12.9 mag. fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.6 (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.eyAJbu1z88 (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3597, passed=30002
Got 30002 stars (including 26372 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 30002 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5133 through 0 to 15.4425, gap 15.4425 to 345.5133
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5133 through 0 to 15.4430, gap 15.4430 to 345.5133
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 29067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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.iIfWG2uMZc (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3594, passed=29935
Got 29935 stars (including 26317 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 29935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4614 through 0 to 15.4602, gap 15.4602 to 345.4614
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4615 through 0 to 15.4618, gap 15.4618 to 345.4615
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 28976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.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.4Fr8T20Kpv (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=252, passed=5959
Got 5959 stars (including 5702 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat
util/solve_plate_with_UCAC5 got 5959 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5281 through 0 to 15.2172, gap 15.2172 to 345.5281
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5280 through 0 to 15.2175, gap 15.2175 to 345.5280
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
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(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits -region wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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.4WXlAxesbP (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=186, passed=5057
Got 5057 stars (including 4869 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat
util/solve_plate_with_UCAC5 got 5057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5279 through 0 to 14.9057, gap 14.9057 to 345.5279
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.5264 through 0 to 14.9056, gap 14.9056 to 345.5264
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 748 (Dec 47.9 to 59.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits -region wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits'
Saving fully-calibrated image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits'
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits'
Preparing the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51829.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51829_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 51829_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:13:44.20 +49:33:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.89, MAG_FAINT_SEARCH_LIMIT=10.87)GAIADR2_OUTPUT=# 1.873 392937216360749312 003.43397522779 +49.55886622792 9.2242 9.0689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51852_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 51852_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:15:50.53 +57:32:39.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cas-04-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
SExtractor catalog cache: saved Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat to cache
SExtractor catalog cache: saved Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Creating symlink local_wcs_cache/wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits exists and is non-empty
wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits exists and is non-empty
wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits exists and is non-empty
wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.845 +53:59:35.63
Second-epoch image center 23:59:31.229 +53:58:21.05
Angular distance between the image centers 0.0778 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 00:00:01.845 +53:59:35.63
Second-epoch image center 23:59:33.992 +53:58:24.31
Angular distance between the image centers 0.0711 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 23:59:31.229 +53:58:21.05
Second-epoch second image center 23:59:33.992 +53:58:24.31
Angular distance between the image centers 0.00683 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/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits &> /tmp/tmp.TpXdjHyjQ2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits &> /tmp/tmp.LK2i7ZQGer
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits &> /tmp/tmp.n5VIjsMVQp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits &> /tmp/tmp.7kq6EU33bi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
Found non-empty wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits and wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
The reference image (wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits) and catalog (wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat) found
'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat' -> 'wcsmag.cat'
Read 205184 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0002 to 359.9998 deg, Dec +47.6490 to +59.3741 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 0.0002 to 359.9998 deg, Dec 47.6490 to 59.3741 deg
Loaded 163418 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): 11964 out of 18942 total matches.
Matched with Tycho-2 18942 out of 205184 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.778547
a=0.000000 b=1.000000 c=22.778547
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 109 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
2.2 pix Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
2.3 pix fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
2.5 pix fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Limiting magnitude estimates:
15.1 mag. Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
15.1 mag. Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
13.3 mag. fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
13.2 mag. fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (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.TpXdjHyjQ2 (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits' -> 'wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=77, blended=35015, passed=205107
Got 205107 stars (including 169770 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 205107 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4449 through 0 to 15.4823, gap 15.4823 to 345.4449
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 201081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4447 through 0 to 15.4832, gap 15.4832 to 345.4447
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.6 to 59.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 201083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 201083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits -region wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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.LK2i7ZQGer (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits' -> 'wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS_IMAGE_NAME=wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS-calibrated image found: wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Checking if the catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits alredy exist and is non-empty...
Catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat corresponding to the image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
WCS catalog name: wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=66, blended=35112, passed=204979
Got 204979 stars (including 169544 good ones) from the SExtractor catalog wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat
util/solve_plate_with_UCAC5 got 204979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4567 through 0 to 15.5151, gap 15.5151 to 345.4567
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 201021 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4571 through 0 to 15.5171, gap 15.5171 to 345.4571
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 201022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 201020 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits -region wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.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.n5VIjsMVQp (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2557, passed=56662
Got 56662 stars (including 54036 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat
util/solve_plate_with_UCAC5 got 56662 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3964 through 0 to 15.3072, gap 15.3072 to 345.3964
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
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(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 54311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.3950 through 0 to 15.3074, gap 15.3074 to 345.3950
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
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(), 54308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 54308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits -region wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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.7kq6EU33bi (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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS_IMAGE_NAME=wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS-calibrated image found: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Checking if the catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat corresponding to the image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
WCS catalog name: wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1726, passed=43647
Got 43647 stars (including 41879 good ones) from the SExtractor catalog wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat
util/solve_plate_with_UCAC5 got 43647 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010469 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4142 through 0 to 15.2715, gap 15.2715 to 345.4142
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 41114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 345.4128 through 0 to 15.2708, gap 15.2708 to 345.4128
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.8 to 59.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 41116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 41116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits -region wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_Cas-04-Q1b1x1_2025-12-26_19-59-31_20.00sec_-15.00C_LIGHT_0057.fits
Saving fully-calibrated image wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_Cas-04-Q1b1x1_2025-12-26_20-00-49_20.00sec_-15.00C_LIGHT_0058.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-11-23_20.00sec_-4.90C_LIGHTs_0237.fits
Saving fully-calibrated image wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.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_Cas-04-Q1b1x1_061329_TTUQ1b1x1_24642_tvqr8ylI/wcs_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238.fits
Preparing the HTML report for the field Cas-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out122924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234234_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 234234_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234235_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234235_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:52:02.75 +53:14:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.614 1945394926946625152 358.01153799969 +53.24694143041 13.0070 12.1607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234249_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234249_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:01:48.55 +50:15:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234262_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234262_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:06:20.88 +56:11:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234264_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234264_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:12:53.14 +53:51:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234267_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234267_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:05:09.46 +57:54:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234271_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234271_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:11:10.93 +55:04:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234277_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234277_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:56:40.52 +56:13:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.595 423605619325774720 014.16959344480 +56.22646621549 11.5813 10.7045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234280_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234280_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:08:51.21 +55:35:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234283_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234283_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:36:32.75 +50:40:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234284_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234284_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:27:16.80 +49:33:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234285_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234285_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:53:12.46 +56:15:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234287_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234287_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:06:27.18 +56:30:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234333_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234333_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:46:04.41 +55:19:40.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234346_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234346_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:15:05.82 +52:39:20.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234362_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234362_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:21:20.61 +51:21:39.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234375_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234375_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:50:13.63 +52:52:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 1.267 1945334144568057728 357.55718452346 +52.87823982723 11.9394 11.2360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234377_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234377_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:57:06.05 +56:45:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234380_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234380_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:38:18.52 +57:32:29.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234385_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234385_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:49:24.21 +55:38:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.224 1994851647159330688 357.34979051894 +55.64963688581 11.9346 11.2710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234390_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234390_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:58:33.48 +51:21:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234393_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234393_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:19:43.34 +55:41:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234404_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234404_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:29:58.21 +49:07:23.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234405_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234405_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:07:13.93 +54:46:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234421_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234421_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:06:36.22 +58:54:21.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234422_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234422_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:46:49.53 +58:40:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234424_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234424_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:28:12.79 +55:15:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 0.731 421149997539215104 007.05302775961 +55.25399733606 12.0997 11.3525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234426_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234426_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:13:50.29 +55:18:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234434_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234434_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:24:13.08 +57:39:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234435_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234435_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:17:09.18 +54:58:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234436_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234436_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:39:37.37 +57:07:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234440_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234440_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:12:15.44 +57:19:00.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234443_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234443_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:26:28.89 +56:07:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234445_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234445_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:02:37.13 +58:27:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.359 422748515649587584 000.65410947493 +58.46575764350 12.5075 11.9333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234450_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234450_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:26:09.86 +55:42:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234452_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234452_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:14:58.11 +53:15:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 2.847 419247086512438528 003.74344618498 +53.25000947936 9.9704 8.4038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234457_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234457_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:16:30.20 +53:57:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.246 419383112417104512 004.12609995604 +53.96563154436 12.4224 11.7114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234461_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234461_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:23:03.57 +55:45:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234466_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234466_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:09:22.65 +57:39:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234480_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234480_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:36:45.96 +56:07:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234489_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234489_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:30:04.73 +49:06:54.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234498_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234498_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:50:40.06 +53:33:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234505_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234505_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:35:26.58 +52:16:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.153 1992966190875060864 353.86030775682 +52.27071739273 12.3794 11.9983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234506_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234506_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:04:20.29 +49:19:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234507_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234507_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:26:27.41 +56:05:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234510_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234510_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:49:08.48 +57:06:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234511_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234511_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:31:46.92 +56:53:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.831 421799426653330176 007.94643128011 +56.89371678961 12.6191 12.0839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234516_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234516_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:47:37.89 +58:01:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234528_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234528_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:59:23.75 +50:31:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234539_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234539_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:36:06.89 +57:18:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234541_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234541_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:33:21.84 +53:58:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 5.116 418060747826239360 008.34340985171 +53.97681218176 12.2031 11.3919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234543_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234543_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:45:47.88 +56:44:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234557_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234557_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:31:20.76 +49:29:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.503 1942918929837476352 352.83599075603 +49.49766204556 12.6241 12.0772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234560_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234560_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:24:36.69 +56:59:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234564_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234564_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:30:01.09 +49:06:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 234575_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234575_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:41:58.41 +50:42:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234578_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234578_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:38:16.64 +57:31:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 4.201 424809064854874880 009.57030182328 +57.52892751200 12.6144 12.1124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234581_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234581_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:36:46.37 +56:08:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.538 418712792577304960 009.19364443735 +56.14032369210 12.6989 12.2667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234607_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234607_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:59:14.62 +53:20:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.877 1945267349237640576 359.81209154784 +53.34320045687 13.2296 12.6291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234621_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234621_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:06:03.23 +49:37:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234631_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234631_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:59:13.03 +53:28:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234632_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234632_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:41:44.24 +52:43:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234637_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234637_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:07:40.90 +53:33:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234640_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234640_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:59:07.03 +53:34:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.059 1945464883374122368 359.77886285924 +53.57856424568 13.1129 12.6082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234645_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234645_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:13:18.21 +57:11:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234647_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234647_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:23:14.35 +53:06:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234648_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234648_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:15:19.72 +53:57:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.077 419385418817918848 003.83206182468 +53.96435238736 12.8761 12.0899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234653_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234653_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:14:15.60 +55:35:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234662_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234662_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:13:37.65 +56:24:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.571 422241464688738688 003.40655329956 +56.41278050306 13.0683 12.4646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234673_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234673_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:18:13.84 +55:28:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234674_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234674_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:22:07.54 +56:34:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234689_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234689_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:01:21.51 +51:12:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234696_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234696_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:15:12.62 +52:38:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234705_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234705_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:59:18.62 +50:33:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234709_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234709_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:08:30.63 +54:41:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234714_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234714_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:05:29.16 +56:23:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234737_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234737_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:57:59.35 +50:26:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.812 1940954514877799936 359.49708375012 +50.43870626711 12.9690 12.5556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234753_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234753_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:02:19.82 +50:28:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234769_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234769_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:05:04.34 +56:02:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.243 420868763081458816 001.26899613369 +56.04744172570 13.2215 12.6026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234770_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234770_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:57:58.51 +50:27:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234830_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234830_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:05:04.85 +51:10:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234842_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234842_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:47:11.49 +51:33:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234859_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234859_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 234860_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 234860_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:52:38.65 +54:21:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92322_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 92322_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 81544_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 81544_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 122924_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 122924_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:17:41.29 +53:02:25.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.33, MAG_FAINT_SEARCH_LIMIT=12.31)
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Considering the candidate 49061_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 49061_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:52:38.65 +56:44:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128312_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 128312_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:49:31.49 +53:08:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110533_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 110533_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 30639_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 30639_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:10:48.49 +57:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72552_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 72552_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 78284_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 78284_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 66326_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 66326_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 111302_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 111302_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:47:01.30 +53:57:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115746_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 115746_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 23:55:48.88 +53:43:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138140_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 138140_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 149329_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 149329_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:07:28.74 +51:52:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101524_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 101524_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 20984_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 20984_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 62822_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 62822_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 71043_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 71043_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 217773_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 217773_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:15:50.53 +57:32:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99160_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 99160_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 41118_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 41118_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
**** FOUND 00:02:19.77 +57:02:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199448_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
Preparing report for the candidate 199448_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
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Considering the candidate 65926_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238
The candidate 65926_fd_Cas-04-Q1b1x1_2026-04-13_06-12-27_20.00sec_-5.00C_LIGHTs_0238 did not pass the final checks
