This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14
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 20.4390* 01 11 58.22 +63 39 46.7 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
NSVS J0111584+633946,2461150.9390,12.63,0.05,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 J0111584+633946 20260420.4390 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 01 09 47.29 +63 24 16.2 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
target,2461150.9390,12.85,0.05,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 20260420.4390 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 00 55 01.79 +61 42 33.8 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
Gaia DR3 427459540713657472,2461150.9390,12.62,0.05,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
Gaia DR3 427459540713657472 20260420.4390 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 00 54 50.31 +60 47 55.1 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
ASASSN-V J005450.49+604755.7,2461150.9390,12.46,0.05,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 J005450.49+604755.7 20260420.4390 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 00 54 51.47 +60 51 30.3 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
ASASSN-V J005451.64+605129.3,2461150.9390,12.21,0.05,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 J005451.64+605129.3 20260420.4390 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9390,12.35,0.05,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 20260420.4390 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9390,12.45,0.05,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 20260420.4390 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 01 09 37.91 +63 02 34.0 11.7 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
ASASSN-V J010938.86+630233.3,2461150.9390,11.74,0.05,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 J010938.86+630233.3 20260420.4390 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 01 01 47.96 +62 01 59.3 12.4 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 J010148.13+620200.2,2461150.9390,12.44,0.05,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 J010148.13+620200.2 20260420.4390 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 20.4390* 01 09 10.12 +62 56 17.4 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 J010910.41+625618.5,2461150.9390,12.58,0.05,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 J010910.41+625618.5 20260420.4390 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!
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,2461150.9390,12.38,0.05,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 20260420.4390 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9390,12.40,0.05,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 20260420.4390 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9390,12.28,0.05,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
target 20260420.4390 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
First image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Last image: 2461150.93939013 20.04.2026 10:32:33.307 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.98
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: 11 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): 23822
Objects passed selection criteria: 23627
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 14192.5
Average stars matched: 13785.5 (97.1323 %)
Memory usage VmPeak: 127800 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:37:13 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: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
First image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Last image: 2461150.93939013 20.04.2026 10:32:33.307 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
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: 64 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): 154673
Objects passed selection criteria: 154204
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 97064.2
Average stars matched: 92871 (95.6799 %)
Memory usage VmPeak: 1982240 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 05:44:42 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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
SExtractor catalog cache: saved Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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: 2461150.93867984
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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
Saving wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits to local_wcs_cache/
'wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits'
wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits (1st reference image)
verification OK: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.853 +61:59:36.76 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:18.214 +62:01:22.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 00:00:18.214 +62:01:22.89
Angular distance between the image centers 0.0435 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Image size: 942.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:20.772 +62:00:57.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 00:00:20.772 +62:00:57.02
Angular distance between the image centers 0.0432 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 00:00:18.214 +62:01:22.89
Second-epoch second image center 00:00:20.772 +62:00:57.02
Angular distance between the image centers 0.00876 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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.HCVbg2gfjJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.4g0OT9DVQx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits &> /tmp/tmp.WxmycuWghX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits &> /tmp/tmp.R2SB7IQYVq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
Found non-empty wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
The reference image (wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits) and catalog (wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat) found
'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat' -> 'wcsmag.cat'
Read 25547 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0005 to 359.9978 deg, Dec +55.3501 to +67.4045 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 0.0005 to 359.9978 deg, Dec 55.3501 to 67.4045 deg
Loaded 133072 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): 14110 out of 15859 total matches.
Matched with Tycho-2 15859 out of 25547 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955169
a=0.000000 b=1.000000 c=22.955169
From vast_summary.log: estimated ref. image limiting mag.: -7.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
2.5 pix Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
3.2 pix fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
2.9 pix fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Limiting magnitude estimates:
15.0 mag. Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
15.0 mag. Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
13.7 mag. fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
13.1 mag. fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.HCVbg2gfjJ (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3206, passed=25547
Got 25547 stars (including 22312 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 25547 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 341.2187 through 0 to 19.8663, gap 19.8663 to 341.2187
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
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(), 950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 24870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.2185 through 0 to 19.8666, gap 19.8666 to 341.2185
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
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(), 24870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 24870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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.4g0OT9DVQx (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3160, passed=25477
Got 25477 stars (including 22297 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 25477 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 341.2186 through 0 to 19.8660, gap 19.8660 to 341.2186
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 24335 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.2185 through 0 to 19.8672, gap 19.8672 to 341.2185
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 24333 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 24332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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.WxmycuWghX (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=152, passed=3194
Got 3194 stars (including 3042 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat
util/solve_plate_with_UCAC5 got 3194 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 341.3948 through 0 to 19.6865, gap 19.6865 to 341.3948
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 341.3941 through 0 to 19.6884, gap 19.6884 to 341.3941
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 2978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits -region wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.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.R2SB7IQYVq (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=112, passed=2929
Got 2929 stars (including 2811 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat
util/solve_plate_with_UCAC5 got 2929 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 341.0795 through 0 to 19.5102, gap 19.5102 to 341.0795
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 2716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 341.0786 through 0 to 19.5114, gap 19.5114 to 341.0786
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 2716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 2716 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits -region wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
Saving fully-calibrated image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits'
Preparing the HTML report for the field Cas-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cas-02-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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
SExtractor catalog cache: saved Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits exists and is non-empty
wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits (1st reference image)
verification OK: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:01.853 +61:59:36.76 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 942.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:18.214 +62:01:22.89 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 00:00:18.214 +62:01:22.89
Angular distance between the image centers 0.0435 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Image size: 942.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:20.772 +62:00:57.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 00:00:20.772 +62:00:57.02
Angular distance between the image centers 0.0432 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 00:00:18.214 +62:01:22.89
Second-epoch second image center 00:00:20.772 +62:00:57.02
Angular distance between the image centers 0.00876 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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.GqjECbn85N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.bzcDiOJDCT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits &> /tmp/tmp.7ALir6V4Et
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits &> /tmp/tmp.3HgZY5FzW8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
Found non-empty wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
The reference image (wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits) and catalog (wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat) found
'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat' -> 'wcsmag.cat'
Read 170710 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 360.0000 deg, Dec +55.3116 to +67.4209 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 0.0001 to 360.0000 deg, Dec 55.3116 to 67.4209 deg
Loaded 133731 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): 10993 out of 16914 total matches.
Matched with Tycho-2 16914 out of 170710 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774723
a=0.000000 b=1.000000 c=22.774723
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
2.3 pix Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
2.8 pix fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
2.7 pix fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Limiting magnitude estimates:
15.1 mag. Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
15.1 mag. Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
13.7 mag. fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
12.9 mag. fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.5 (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.GqjECbn85N (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=28495, passed=170667
Got 170667 stars (including 141945 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 170667 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 341.2187 through 0 to 20.1102, gap 20.1102 to 341.2187
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 167931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.2186 through 0 to 20.1103, gap 20.1103 to 341.2186
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 167930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 167935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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.bzcDiOJDCT (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=73, blended=28343, passed=170972
Got 170972 stars (including 142388 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 170972 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 341.2186 through 0 to 20.0818, gap 20.0818 to 341.2186
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 166822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.2184 through 0 to 20.0827, gap 20.0827 to 341.2184
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 166822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 166822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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.7ALir6V4Et (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1093, passed=25277
Got 25277 stars (including 24136 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat
util/solve_plate_with_UCAC5 got 25277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 341.0789 through 0 to 20.0262, gap 20.0262 to 341.0789
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 22638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 341.0791 through 0 to 20.0282, gap 20.0282 to 341.0791
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.4)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 22634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 22633 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits -region wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.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.3HgZY5FzW8 (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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=887, passed=23514
Got 23514 stars (including 22583 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat
util/solve_plate_with_UCAC5 got 23514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 341.0795 through 0 to 20.0273, gap 20.0273 to 341.0795
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.4)
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: 955 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 21117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 341.0788 through 0 to 20.0287, gap 20.0287 to 341.0788
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.6 to 67.4)
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: 955 matched stars entering correct_measured_positions(), 21114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 21114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits -region wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_Cas-02-Q1b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Saving fully-calibrated image wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_Cas-02-Q1b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Saving fully-calibrated image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-31-31_20.00sec_-4.90C_LIGHTs_0022.fits
Saving fully-calibrated image wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.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_2026-04-20_CI_Cas-02-Q1b1x1_053328_TTUQ1b1x1_3327382_p01lak14/wcs_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023.fits
Preparing the HTML report for the field Cas-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out101266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98358.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 25s
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: 7s
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Considering the candidate 196556_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196556_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:57:27.80 +62:06:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196564_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196564_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:48:56.52 +60:40:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196565_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196565_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 23:00:03.96 +59:19:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196567_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196567_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 23:13:48.80 +59:50:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196606_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196606_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 23:03:19.17 +60:26:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196713_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196713_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:54:15.53 +60:34:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196725_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196725_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:53:02.57 +60:35:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196726_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196726_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 01:03:47.01 +61:03:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196800_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196800_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 01:03:36.78 +61:02:59.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196819_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196819_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:53:04.61 +60:00:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196829_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196829_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 00:54:44.94 +61:31:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196875_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196875_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 23:13:30.99 +60:28:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196877_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196877_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 01:01:47.27 +61:46:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196903_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196903_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 01:09:26.72 +62:56:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196922_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 196922_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 23:05:05.11 +58:45:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14492_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 14492_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 18054_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 18054_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 50874_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 50874_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 31779_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 31779_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
**** FOUND 01:01:09.94 +62:41:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66463_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 66463_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 65593_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 65593_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 101266_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 101266_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 101943_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
Preparing report for the candidate 101943_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
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Considering the candidate 53295_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023
The candidate 53295_fd_Cas-02-Q1b1x1_2026-04-20_05-32-33_20.00sec_-4.90C_LIGHTs_0023 did not pass the final checks
