This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,6.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 6.67CV 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
VARIABLE_NAME,2461292.9703,6.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 6.98CV 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
VARIABLE_NAME,2461292.9703,7.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,7.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,7.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,7.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.17CV 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
VARIABLE_NAME,2461292.9703,7.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,7.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 7.40CV 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
Mean magnitude and position on the discovery images:
2026 09 09.4703 2461292.9703 12.68 08:52:30.06 +14:33:45.1
212.84025 33.28505 galactic Cnc Second-epoch detections are separated by 1.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.747 Winchester -0 0 0 13.2 -0 0
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:52:30.06 +14:33:45.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:52:30.06 +14:33:45.1: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 12.68CV 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
Mean magnitude and position on the discovery images:
2026 09 09.4703 2461292.9703 13.43 08:45:51.22 +16:02:51.5
210.47324 32.37991 galactic Cnc Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.584 Semiramis 0 0 1 13.7 -0 0
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:45:51.22 +16:02:51.5: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:45:51.22 +16:02:51.5: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 13.43CV 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
Mean magnitude and position on the discovery images:
2026 09 09.4703 2461292.9703 11.79 08:52:16.53 +16:30:46.8
210.65158 33.98278 galactic Cnc Second-epoch detections are separated by 0.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.52 Europa 0 0 0 12.3 0 0
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:52:16.53 +16:30:46.8: 14.55 +/- 0.08 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:52:16.53 +16:30:46.8: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.06
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461292.9703,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260909.4703 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
First image: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Last image: 2461292.97063446 09.09.2026 11:17:32.817 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8231
Objects passed selection criteria: 8219
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 5608.75
Average stars matched: 5269 (93.9425 %)
Memory usage VmPeak: 234884 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 06:23:10 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: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
First image: 2461093.74344014 22.02.2026 05:50:23.228 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Last image: 2461292.97063446 09.09.2026 11:17:32.817 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 48412
Objects passed selection criteria: 48260
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 34242
Average stars matched: 31821.5 (92.9312 %)
Memory usage VmPeak: 269964 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Sep 9 06:24:00 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.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/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.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: 2461292.97002484
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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (1st reference image)
verification OK: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:53:21.014 +14:00:00.07 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 939.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:14.164 +13:59:55.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:14.164 +13:59:55.12
Angular distance between the image centers 0.0277 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Image size: 939.6'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:12.619 +13:59:26.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:12.619 +13:59:26.54
Angular distance between the image centers 0.0352 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 08:53:14.164 +13:59:55.12
Second-epoch second image center 08:53:12.619 +13:59:26.54
Angular distance between the image centers 0.01010 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.6AhTpNHa8G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.FXKxeaelMB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.BXkrAvcQVM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits &> /tmp/tmp.aAjajTrKhn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat) found
'wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat' -> 'wcsmag.cat'
Read 12501 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0576 to 141.9546 deg, Dec +8.1318 to +19.6232 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 125.0576 to 141.9546 deg, Dec 8.1318 to 19.6232 deg
Loaded 7593 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): 5630 out of 5966 total matches.
Matched with Tycho-2 5966 out of 12501 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.977100
a=0.000000 b=1.000000 c=22.977100
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12501 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0576 to 141.9546 deg, Dec +8.1318 to +19.6232 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 125.0576 to 141.9546 deg, Dec 8.1318 to 19.6232 deg
Loaded 7593 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): 5630 out of 5966 total matches.
Matched with Tycho-2 5966 out of 12501 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -> calib.txt_param_ref_wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (aperture=6.5)
Read 9951 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0604 to 141.9546 deg, Dec +8.1147 to +19.5889 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 125.0604 to 141.9546 deg, Dec 8.1147 to 19.5889 deg
Loaded 7587 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): 5641 out of 5952 total matches.
Matched with Tycho-2 5952 out of 9951 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -> calib.txt_param_ref_wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
2.2 pix Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
2.3 pix fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
2.3 pix fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Limiting magnitude estimates:
15.4 mag. Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
15.2 mag. Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
13.7 mag. fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
13.7 mag. fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.9 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.6AhTpNHa8G (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=855, bad_region=3640, passed=12501
Got 12501 stars (including 8254 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 12501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 9591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 9591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 9591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits N_match=4868 sigma_overall_arcsec=0.318 sigma_q1_arcsec=0.279 sigma_q2_arcsec=0.355 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.323 n_q1=1409 n_q2=1070 n_q3=1301 n_q4=1088 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FXKxeaelMB (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, bad_region=2628, passed=9951
Got 9951 stars (including 6771 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 9951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 4862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4862 matched stars entering correct_measured_positions(), 7875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 7875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4861 matched stars entering correct_measured_positions(), 7875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4861 stars left (next iteration limit 5348)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits N_match=4861 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.307 sigma_q4_arcsec=0.312 n_q1=1383 n_q2=1001 n_q3=1399 n_q4=1078 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.BXkrAvcQVM (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=256, bad_region=597, passed=3806
Got 3806 stars (including 2989 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 3806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2908 matched stars entering correct_measured_positions(), 2907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2908 matched stars entering correct_measured_positions(), 3291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2909 matched stars entering correct_measured_positions(), 3291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 2909 matched stars entering correct_measured_positions(), 3291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 2909 stars left (next iteration limit 3198)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2909 robust_rms=5.561 arcsec worst_quadrant_rms=16.915 arcsec
SIP_REFIT: SIP order 3 trial: matched=2909 robust_rms=0.643 arcsec worst_quadrant_rms=0.676 arcsec
SIP_REFIT: SIP order 5 trial: matched=2909 robust_rms=0.486 arcsec worst_quadrant_rms=0.507 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2909 robust_rms_before=1.257 arcsec robust_rms_before_corrected=0.463 arcsec robust_rms_after=0.486 arcsec worst_quadrant_rms_before=0.476 worst_quadrant_rms_after=0.507
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.476 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits N_match=2909 sigma_overall_arcsec=0.474 sigma_q1_arcsec=0.454 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.498 sigma_q4_arcsec=0.500 n_q1=1072 n_q2=334 n_q3=1083 n_q4=420 worst_quadrant_to_overall_ratio=1.056
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.aAjajTrKhn (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=288, bad_region=631, passed=3790
Got 3790 stars (including 2949 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat
util/solve_plate_with_UCAC5 got 3790 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.6'
Seting catalog search parameters based on the expected field of view 939.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013050 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010440 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2871 matched stars entering correct_measured_positions(), 2871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2871 matched stars entering correct_measured_positions(), 3241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2873 matched stars entering correct_measured_positions(), 3241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 2873 matched stars entering correct_measured_positions(), 3241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 2873 stars left (next iteration limit 3158)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2873 robust_rms=5.517 arcsec worst_quadrant_rms=17.156 arcsec
SIP_REFIT: SIP order 3 trial: matched=2873 robust_rms=0.631 arcsec worst_quadrant_rms=0.670 arcsec
SIP_REFIT: SIP order 5 trial: matched=2873 robust_rms=0.474 arcsec worst_quadrant_rms=0.503 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2873 robust_rms_before=1.245 arcsec robust_rms_before_corrected=0.456 arcsec robust_rms_after=0.474 arcsec worst_quadrant_rms_before=0.464 worst_quadrant_rms_after=0.503
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.464 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits N_match=2873 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.444 sigma_q3_arcsec=0.507 sigma_q4_arcsec=0.445 n_q1=1064 n_q2=331 n_q3=1077 n_q4=401 worst_quadrant_to_overall_ratio=1.088
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
Saving the final (post-refit) wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
Saving the final (post-refit) wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits'
Saving the final (post-refit) wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits sigma_overall=0.318 worst_q_ratio=1.119
ref2=Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits sigma_overall=0.352 worst_q_ratio=1.218
new1=fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits sigma_overall=0.474 worst_q_ratio=1.056
new2=fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits sigma_overall=0.466 worst_q_ratio=1.088
reference average sigma_overall=0.335 worst_q_ratio=1.1685
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187_astrometric_residuals.png (4868 matched stars from wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114_astrometric_residuals.png (4861 matched stars from wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401_astrometric_residuals.png (2909 matched stars from wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402_astrometric_residuals.png (2873 matched stars from wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits'
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20148_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 20148_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20153_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 20153_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20156_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 20156_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20160_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 20160_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (1st reference image)
verification OK: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 08:53:21.014 +14:00:00.07 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Image size: 939.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:14.164 +13:59:55.12 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:14.164 +13:59:55.12
Angular distance between the image centers 0.0277 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Image size: 939.6'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:12.619 +13:59:26.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:21.014 +14:00:00.07
Second-epoch image center 08:53:12.619 +13:59:26.54
Angular distance between the image centers 0.0352 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 08:53:14.164 +13:59:55.12
Second-epoch second image center 08:53:12.619 +13:59:26.54
Angular distance between the image centers 0.01010 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits &> /tmp/tmp.M4V44ake0Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits &> /tmp/tmp.PxjxnqIzZv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits &> /tmp/tmp.hKasGLQq5J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits &> /tmp/tmp.lmpZMKLNv1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits and wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat) found
'wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat' -> 'wcsmag.cat'
Read 63179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0577 to 141.9546 deg, Dec +8.1206 to +19.6320 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 125.0577 to 141.9546 deg, Dec 8.1206 to 19.6320 deg
Loaded 7608 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): 5179 out of 5984 total matches.
Matched with Tycho-2 5984 out of 63179 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858100
a=0.000000 b=1.000000 c=22.858100
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 63179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0577 to 141.9546 deg, Dec +8.1206 to +19.6320 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 125.0577 to 141.9546 deg, Dec 8.1206 to 19.6320 deg
Loaded 7608 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): 5179 out of 5984 total matches.
Matched with Tycho-2 5984 out of 63179 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -> calib.txt_param_ref_wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (aperture=5.1)
Read 59553 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.0604 to 141.9546 deg, Dec +8.1147 to +19.5889 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 125.0604 to 141.9546 deg, Dec 8.1147 to 19.5889 deg
Loaded 7587 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): 5243 out of 6043 total matches.
Matched with Tycho-2 6043 out of 59553 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Forced-photometry filter: calibrated wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -> calib.txt_param_ref_wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
2.0 pix Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
2.1 pix fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
2.1 pix fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Limiting magnitude estimates:
15.6 mag. Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
15.4 mag. Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
13.9 mag. fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
13.9 mag. fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.M4V44ake0Z (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits 566.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=4250, bad_region=14474, passed=63156
Got 63156 stars (including 45591 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 63156 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 52207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4878 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 52207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 52207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits N_match=4873 sigma_overall_arcsec=0.308 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.335 sigma_q4_arcsec=0.300 n_q1=1451 n_q2=1071 n_q3=1301 n_q4=1050 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits -region wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.PxjxnqIzZv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3477, bad_region=15002, passed=59531
Got 59531 stars (including 41920 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 59531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 4855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4855 matched stars entering correct_measured_positions(), 47769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 47769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 47769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4854 stars left (next iteration limit 5340)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits N_match=4854 sigma_overall_arcsec=0.331 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.291 n_q1=1398 n_q2=979 n_q3=1412 n_q4=1065 worst_quadrant_to_overall_ratio=1.230
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits -region wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.hKasGLQq5J (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=873, bad_region=2991, passed=25551
Got 25551 stars (including 21740 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat
util/solve_plate_with_UCAC5 got 25551 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.7'
Seting catalog search parameters based on the expected field of view 939.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013051 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010441 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 23278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 23278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 23278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 4865 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4865 robust_rms=5.508 arcsec worst_quadrant_rms=16.841 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.665 arcsec worst_quadrant_rms=0.699 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.497 arcsec worst_quadrant_rms=0.554 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=1.264 arcsec robust_rms_before_corrected=0.469 arcsec robust_rms_after=0.497 arcsec worst_quadrant_rms_before=0.503 worst_quadrant_rms_after=0.554
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.503 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits N_match=4865 sigma_overall_arcsec=0.476 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.493 sigma_q3_arcsec=0.500 sigma_q4_arcsec=0.464 n_q1=1861 n_q2=636 n_q3=1660 n_q4=708 worst_quadrant_to_overall_ratio=1.051
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.lmpZMKLNv1 (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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=10, blended=876, bad_region=2968, passed=25130
Got 25130 stars (including 21381 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat
util/solve_plate_with_UCAC5 got 25130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.6'
Seting catalog search parameters based on the expected field of view 939.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013050 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010440 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4879 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 22860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4877 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 22860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 22860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 4870 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4870 robust_rms=5.454 arcsec worst_quadrant_rms=18.312 arcsec
SIP_REFIT: SIP order 3 trial: matched=4870 robust_rms=0.638 arcsec worst_quadrant_rms=0.675 arcsec
SIP_REFIT: SIP order 5 trial: matched=4870 robust_rms=0.483 arcsec worst_quadrant_rms=0.506 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4870 robust_rms_before=1.255 arcsec robust_rms_before_corrected=0.462 arcsec robust_rms_after=0.483 arcsec worst_quadrant_rms_before=0.486 worst_quadrant_rms_after=0.506
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.486 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits N_match=4870 sigma_overall_arcsec=0.467 sigma_q1_arcsec=0.449 sigma_q2_arcsec=0.474 sigma_q3_arcsec=0.491 sigma_q4_arcsec=0.441 n_q1=1860 n_q2=642 n_q3=1660 n_q4=708 worst_quadrant_to_overall_ratio=1.051
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-16-40_20.00sec_-0.00C_LIGHT_0401.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.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_2026-09-09_CI_Cnc-05-Q2b1x1_062053_TTUQ2b1x1_1308875_2ft1GTHY/wcs_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402.fits
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:51:20.12 +11:46:42.1: 12.30 +/- 0.04 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:50:18.88 +09:45:07.9: 12.94 +/- 0.02 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:51:15.59 +11:50:55.2: 12.28 +/- 0.02 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:47:44.87 +13:18:59.8: 12.59 +/- 0.01 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:01:28.70 +11:19:40.6: 13.11 +/- 0.02 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:51:23.97 +11:48:21.4: 12.05 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:01:28.70 +11:19:40.6: 13.14 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:51:23.97 +11:48:21.4: 12.16 +/- 0.04 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:47:44.87 +13:18:59.8: 12.64 +/- 0.01 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:51:20.12 +11:46:42.1: 12.42 +/- 0.05 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:50:18.88 +09:45:07.9: 13.04 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:51:15.59 +11:50:55.2: 12.39 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry reference-image weighted average: 12.09 +/- 0.02
Forced photometry reference-image weighted average: 12.34 +/- 0.03
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry reference-image weighted average: 12.98 +/- 0.02
Forced photometry reference-image weighted average: 12.32 +/- 0.01
Forced photometry filter REJECTED candidate at 09:01:28.70 +11:19:40.6: ref_mag=13.12 +/- 0.02 new_mean_mag=13.2961 delta=-0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:51:23.97 +11:48:21.4: ref_mag=12.09 +/- 0.02 new_mean_mag=12.2720 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:47:44.87 +13:18:59.8: ref_mag=12.61 +/- 0.01 new_mean_mag=12.8818 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:51:20.12 +11:46:42.1: ref_mag=12.34 +/- 0.03 new_mean_mag=12.6080 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:50:18.88 +09:45:07.9: ref_mag=12.98 +/- 0.02 new_mean_mag=13.2476 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:51:15.59 +11:50:55.2: ref_mag=12.32 +/- 0.01 new_mean_mag=12.4619 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:52:30.06 +14:33:45.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:51:17.37 +11:47:00.4: 12.82 +/- 0.06 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:48:32.51 +10:25:10.3: 12.60 +/- 0.02 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:52:30.06 +14:33:45.1: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:51:17.37 +11:47:00.4: 13.01 +/- 0.09 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:48:32.51 +10:25:10.3: 12.47 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.88 +/- 0.05
Forced photometry filter REJECTED candidate at 08:51:17.37 +11:47:00.4: ref_mag=12.88 +/- 0.05 new_mean_mag=12.8339 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry filter REJECTED candidate at 08:48:32.51 +10:25:10.3: ref_mag=12.54 +/- 0.01 new_mean_mag=12.5158 delta=0.02 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:47:33.83 +10:39:19.9: 13.19 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 09:08:09.53 +14:41:27.3: 13.09 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:47:33.83 +10:39:19.9: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:45:51.22 +16:02:51.5: 16.18 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.20 +/- 0.02
Forced photometry filter REJECTED candidate at 08:47:33.83 +10:39:19.9: ref_mag=13.20 +/- 0.02 new_mean_mag=13.0039 delta=0.19 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:51:22.06 +11:46:40.3: 13.09 +/- 0.09 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 09:08:09.53 +14:41:27.3: 13.08 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter REJECTED candidate at 09:08:09.53 +14:41:27.3: ref_mag=13.09 +/- 0.02 new_mean_mag=13.1646 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-02-21_23-50-23_20.00sec_-15.00C_LIGHT_0187.fits at 08:52:16.53 +16:30:46.8: 14.55 +/- 0.08 detection
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:45:51.22 +16:02:51.5: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:51:22.06 +11:46:40.3: 13.13 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.07
Forced photometry filter REJECTED candidate at 08:51:22.06 +11:46:40.3: ref_mag=13.10 +/- 0.07 new_mean_mag=13.1483 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Cnc-05-Q2b1x1_2026-04-15_23-32-43_20.00sec_-4.90C_LIGHTs_0114.fits at 08:52:16.53 +16:30:46.8: 14.63 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.58 +/- 0.06
Forced photometry filter KEPT candidate at 08:52:16.53 +16:30:46.8: ref_mag=14.58 +/- 0.06 new_mean_mag=11.7906 delta=2.79 (need > 0.90)
Adding exclusion_list_local.txt__out15063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80919.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 4s
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Considering the candidate 75320_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75320_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75322_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75322_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75323_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75323_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75324_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75324_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75325_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75325_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75326_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75326_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:51:18.68 +11:47:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75327_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 75327_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 75335_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 75335_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 75336_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 75336_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 75340_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 75340_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 75345_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 75345_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 78209_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 78209_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 78508_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 78508_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:51:25.86 +11:49:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78525_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 78525_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 09:08:21.05 +13:11:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78571_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 78571_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 78691_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 78691_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:44:40.00 +10:06:16.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79110_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79110_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 79380_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79380_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:43:45.50 +11:14:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79577_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79577_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:51:20.75 +11:45:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79629_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79629_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:46:55.62 +12:05:11.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79632_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79632_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 79686_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 79686_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:49:32.78 +12:08:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80068_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 80068_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 09:10:21.05 +13:22:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80349_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 80349_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 80495_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 80495_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
**** FOUND 08:43:08.97 +14:05:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80750_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 80750_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
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Considering the candidate 80919_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
Preparing report for the candidate 80919_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
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Considering the candidate 06362_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402
The candidate 06362_fd_Cnc-05-Q2b1x1_2026-09-09_06-17-32_20.00sec_-0.00C_LIGHT_0402 did not pass the final checks
