This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU
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,2461323.8489,6.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 6.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 11.02 08:21:33.74 +19:25:58.1
204.35807 28.24928 galactic Cnc Second-epoch detections are separated by 1.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.27 Euterpe 0 -0 0 11.2 0 -0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:21:33.74 +19:25:58.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:21:33.74 +19:25:58.1: 15.90 +/- 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,2461323.8489,11.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 11.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 11.80 08:09:41.11 +21:17:41.4
201.28509 26.31091 galactic Cnc Second-epoch detections are separated by 0.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.30 Urania 0 1 1 12.2 0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:09:41.11 +21:17:41.4: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:09:41.11 +21:17:41.4: 15.96 +/- 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,2461323.8489,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 11.80CV 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,2461323.8489,6.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 6.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 12.91 08:21:18.14 +21:45:41.1
201.84838 29.00677 galactic Cnc Second-epoch detections are separated by 1.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.111 Ate 0 -0 1 13.1 -0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:21:18.14 +21:45:41.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:21:18.14 +21:45:41.1: 16.18 +/- 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,2461323.8489,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 13.19 08:38:34.50 +25:23:05.9
199.27972 33.90475 galactic Cnc Second-epoch detections are separated by 1.4" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.423 Diotima 1 -0 1 13.4 0 -0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:38:34.50 +25:23:05.9: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:38:34.50 +25:23:05.9: 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,2461323.8489,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 13.67 07:57:54.80 +23:50:13.9
197.59481 24.65213 galactic Gem Second-epoch detections are separated by 0.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.579 Sidonia 0 0 1 14.0 0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:57:54.80 +23:50:13.9: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 07:57:54.80 +23:50:13.9: 16.09 +/- 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,2461323.8489,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 13.67CV 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
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 13.59 08:16:58.68 +19:54:45.2
203.41375 27.41415 galactic Cnc Second-epoch detections are separated by 2.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.779 Nina 1 -0 1 13.7 0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:16:58.68 +19:54:45.2: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:16:58.68 +19:54:45.2: 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,2461323.8489,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 13.59CV 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 10 10.3489 2461323.8489 13.78 08:05:21.00 +20:16:02.2
201.94589 24.99646 galactic Cnc Second-epoch detections are separated by 2.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.171 Ophelia 1 -0 1 14.2 0 0
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:05:21.00 +20:16:02.2: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:05:21.00 +20:16:02.2: 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,2461323.8489,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261010.3489 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 10.3489 2461323.8489 9.71 08:28:24.87 +19:35:44.9
204.84242 29.81590 galactic Cnc Second-epoch detections are separated by 0.8" and 7.0 pix
The object was found in VSX 0" ASAS J082825+1935.7
Type: MISC
# Max. Min./Amp. JD0 Period
10.850 V Y 0.330 V 2452811.70000 71.018865000000 M6
The object was not found in astcheck.
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:28:24.87 +19:35:44.9: 10.66 +/- 0.00 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:28:24.87 +19:35:44.9: 10.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.00
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
ASAS J082825+1935.7,2461323.8489,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J082825+1935.7 20261010.3489 9.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
First image: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Last image: 2461323.84919784 10.10.2026 08:22:40.693 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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): 12836
Objects passed selection criteria: 12813
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 10719.8
Average stars matched: 10338 (96.4388 %)
Memory usage VmPeak: 238652 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Oct 10 04:38:35 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: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
First image: 2461093.70071369 22.02.2026 04:48:51.663 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Last image: 2461323.84919784 10.10.2026 08:22:40.693 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.00
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: 20 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): 72729
Objects passed selection criteria: 72559
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 58827.5
Average stars matched: 57290.5 (97.3873 %)
Memory usage VmPeak: 560408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Oct 10 04:39:46 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461323.84854862
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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (1st reference image)
verification OK: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:25.612 +22:00:41.04 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Image size: 943.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:26.106 +21:58:42.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:25.612 +22:00:41.04
Second-epoch image center 08:18:26.106 +21:58:42.16
Angular distance between the image centers 0.0331 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Image size: 943.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:26.968 +21:58:01.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:25.612 +22:00:41.04
Second-epoch image center 08:18:26.968 +21:58:01.07
Angular distance between the image centers 0.0447 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 08:18:26.106 +21:58:42.16
Second-epoch second image center 08:18:26.968 +21:58:01.07
Angular distance between the image centers 0.01189 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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.s612M92G1w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits &> /tmp/tmp.qRQgnNrOhG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits &> /tmp/tmp.NC5NT160m5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits &> /tmp/tmp.1uul4rUmVJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat' -> 'wcsmag.cat'
Read 13640 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6688 to 133.2139 deg, Dec +16.3184 to +27.3542 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 115.6688 to 133.2139 deg, Dec 16.3184 to 27.3542 deg
Loaded 8750 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): 6703 out of 7196 total matches.
Matched with Tycho-2 7196 out of 13640 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.927500
a=0.000000 b=1.000000 c=22.927500
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 13640 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6688 to 133.2139 deg, Dec +16.3184 to +27.3542 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 115.6688 to 133.2139 deg, Dec 16.3184 to 27.3542 deg
Loaded 8750 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): 6703 out of 7196 total matches.
Matched with Tycho-2 7196 out of 13640 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (aperture=6.2)
Read 13884 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.9226 to 133.4579 deg, Dec +16.5877 to +27.2909 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 115.9226 to 133.4579 deg, Dec 16.5877 to 27.2909 deg
Loaded 8367 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): 6692 out of 7091 total matches.
Matched with Tycho-2 7091 out of 13884 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.4 pix Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
3.0 pix fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
3.0 pix fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Limiting magnitude estimates:
15.6 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.5 mag. Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
14.5 mag. fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
14.5 mag. fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.s612M92G1w (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=1109, bad_region=0, passed=13640
Got 13640 stars (including 12518 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
util/solve_plate_with_UCAC5 got 13640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 4925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 13640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 13640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 13640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4925 stars left (next iteration limit 5417)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits N_match=4925 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.324 sigma_q3_arcsec=0.326 sigma_q4_arcsec=0.285 n_q1=1290 n_q2=1207 n_q3=1346 n_q4=1082 worst_quadrant_to_overall_ratio=1.291
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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.qRQgnNrOhG (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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=1000, bad_region=0, passed=13884
Got 13884 stars (including 12872 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 13884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 13884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 13884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 13884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4920 stars left (next iteration limit 5412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits N_match=4920 sigma_overall_arcsec=0.336 sigma_q1_arcsec=0.283 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.367 n_q1=1046 n_q2=1412 n_q3=1116 n_q4=1346 worst_quadrant_to_overall_ratio=1.204
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits -region wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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.NC5NT160m5 (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=340, bad_region=0, passed=7794
Got 7794 stars (including 7447 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat
util/solve_plate_with_UCAC5 got 7794 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 7794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4910 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4910 robust_rms=10.409 arcsec worst_region_rms=27.232 arcsec outer_annulus_rms=27.232 arcsec
SIP_REFIT: SIP order 3 trial: matched=4910 robust_rms=0.561 arcsec worst_region_rms=0.808 arcsec outer_annulus_rms=0.808 arcsec
SIP_REFIT: SIP order 5 trial: matched=4910 robust_rms=0.385 arcsec worst_region_rms=0.474 arcsec outer_annulus_rms=0.474 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4910 robust_rms_before=1.150 arcsec robust_rms_before_corrected=0.314 arcsec robust_rms_after=0.385 arcsec worst_region_rms_before=0.462 worst_region_rms_after=0.474 outer_annulus_rms_before=1.320 outer_annulus_rms_after=0.474
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.462 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits worst_region_rms_kept=0.462 arcsec robust_rms_kept=0.314 arcsec matched=4910
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits N_match=4910 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.401 sigma_q3_arcsec=0.250 sigma_q4_arcsec=0.330 n_q1=1476 n_q2=974 n_q3=1517 n_q4=943 worst_quadrant_to_overall_ratio=1.258
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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.1uul4rUmVJ (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=340, bad_region=0, passed=7804
Got 7804 stars (including 7455 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat
util/solve_plate_with_UCAC5 got 7804 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010484 (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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 7804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 7804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 7804 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4913 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4913 robust_rms=10.582 arcsec worst_region_rms=26.731 arcsec outer_annulus_rms=26.731 arcsec
SIP_REFIT: SIP order 3 trial: matched=4913 robust_rms=0.642 arcsec worst_region_rms=0.916 arcsec outer_annulus_rms=0.916 arcsec
SIP_REFIT: SIP order 5 trial: matched=4913 robust_rms=0.420 arcsec worst_region_rms=0.535 arcsec outer_annulus_rms=0.535 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4913 robust_rms_before=1.182 arcsec robust_rms_before_corrected=0.312 arcsec robust_rms_after=0.420 arcsec worst_region_rms_before=0.459 worst_region_rms_after=0.535 outer_annulus_rms_before=1.315 outer_annulus_rms_after=0.535
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.459 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits worst_region_rms_kept=0.459 arcsec robust_rms_kept=0.312 arcsec matched=4913
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits N_match=4913 sigma_overall_arcsec=0.311 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.252 sigma_q4_arcsec=0.344 n_q1=1478 n_q2=975 n_q3=1511 n_q4=949 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
Saving the final (post-refit) wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits'
Saving the final (post-refit) wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits'
Saving the final (post-refit) wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits sigma_overall=0.340 worst_q_ratio=1.291
ref2=Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits sigma_overall=0.336 worst_q_ratio=1.204
new1=fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits sigma_overall=0.319 worst_q_ratio=1.258
new2=fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits sigma_overall=0.311 worst_q_ratio=1.187
reference average sigma_overall=0.338 worst_q_ratio=1.2475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174_astrometric_residuals.png (4925 matched stars from wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166_astrometric_residuals.png (4920 matched stars from wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426_astrometric_residuals.png (4910 matched stars from wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427_astrometric_residuals.png (4913 matched stars from wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits'
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:21:33.74 +19:25:58.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:09:41.11 +21:17:41.4: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:21:33.74 +19:25:58.1: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:09:41.11 +21:17:41.4: 15.96 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out21395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21466.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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21299_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 21299_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21390_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 21390_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:10:29.43 +24:01:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21395_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 21395_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21398_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 21398_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:57:09.53 +21:19:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21466_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 21466_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01460_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 01460_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:44:40.88 +18:09:09.3 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05635_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 05635_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:59:14.46 +20:38:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03388_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 03388_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:27:40.49 +19:15:44.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:21:33.74 +19:25:58.1
08:09:41.11 +21:17:41.4
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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Checking 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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (1st reference image)
verification OK: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:25.612 +22:00:41.04 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Image size: 943.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:26.106 +21:58:42.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:25.612 +22:00:41.04
Second-epoch image center 08:18:26.106 +21:58:42.16
Angular distance between the image centers 0.0331 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Image size: 943.6'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:26.968 +21:58:01.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:25.612 +22:00:41.04
Second-epoch image center 08:18:26.968 +21:58:01.07
Angular distance between the image centers 0.0447 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 08:18:26.106 +21:58:42.16
Second-epoch second image center 08:18:26.968 +21:58:01.07
Angular distance between the image centers 0.01189 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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.u18d7P5tDz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits &> /tmp/tmp.nphjuX5FWO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits &> /tmp/tmp.PdGLH4v4Lp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits &> /tmp/tmp.QpMFB84F0O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat' -> 'wcsmag.cat'
Read 84357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6148 to 133.2139 deg, Dec +16.3184 to +27.3628 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 115.6148 to 133.2139 deg, Dec 16.3184 to 27.3628 deg
Loaded 8803 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): 5955 out of 7248 total matches.
Matched with Tycho-2 7248 out of 84357 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798700
a=0.000000 b=1.000000 c=22.798700
From vast_summary.log: estimated ref. image limiting mag.: -7.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.80
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 84357 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6148 to 133.2139 deg, Dec +16.3184 to +27.3628 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 115.6148 to 133.2139 deg, Dec 16.3184 to 27.3628 deg
Loaded 8803 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): 5955 out of 7248 total matches.
Matched with Tycho-2 7248 out of 84357 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (aperture=4.7)
Read 76309 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.9226 to 133.4579 deg, Dec +16.5873 to +27.2965 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 115.9226 to 133.4579 deg, Dec 16.5873 to 27.2965 deg
Loaded 8372 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): 6050 out of 7125 total matches.
Matched with Tycho-2 7125 out of 76309 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Forced-photometry filter: calibrated wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.2 pix Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
3.0 pix fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
3.0 pix fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Limiting magnitude estimates:
15.8 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.7 mag. Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
14.5 mag. fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
14.5 mag. fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.u18d7P5tDz (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=30, blended=6314, bad_region=5, passed=84327
Got 84327 stars (including 77868 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat
util/solve_plate_with_UCAC5 got 84327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 84327 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 84327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 84327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4920 stars left (next iteration limit 5412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits N_match=4920 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.418 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.269 n_q1=1289 n_q2=1186 n_q3=1331 n_q4=1114 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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.nphjuX5FWO (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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=30, blended=5596, bad_region=1, passed=76279
Got 76279 stars (including 70572 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 76279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 76279 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 4926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 76279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 76279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4920 stars left (next iteration limit 5412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits N_match=4920 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.276 sigma_q2_arcsec=0.409 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.375 n_q1=1078 n_q2=1426 n_q3=1059 n_q4=1357 worst_quadrant_to_overall_ratio=1.209
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits -region wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.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.PdGLH4v4Lp (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=9, blended=1568, bad_region=43, passed=38168
Got 38168 stars (including 36519 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat
util/solve_plate_with_UCAC5 got 38168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.7'
Seting catalog search parameters based on the expected field of view 943.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013107 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010486 (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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 38168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 38168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 38168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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=4912 robust_rms=10.555 arcsec worst_region_rms=26.084 arcsec outer_annulus_rms=26.084 arcsec
SIP_REFIT: SIP order 3 trial: matched=4912 robust_rms=0.563 arcsec worst_region_rms=0.797 arcsec outer_annulus_rms=0.797 arcsec
SIP_REFIT: SIP order 5 trial: matched=4912 robust_rms=0.386 arcsec worst_region_rms=0.470 arcsec outer_annulus_rms=0.470 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4912 robust_rms_before=1.145 arcsec robust_rms_before_corrected=0.314 arcsec robust_rms_after=0.386 arcsec worst_region_rms_before=0.467 worst_region_rms_after=0.470 outer_annulus_rms_before=1.306 outer_annulus_rms_after=0.470
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.467 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits worst_region_rms_kept=0.467 arcsec robust_rms_kept=0.314 arcsec matched=4912
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits N_match=4912 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.346 n_q1=1480 n_q2=942 n_q3=1527 n_q4=963 worst_quadrant_to_overall_ratio=1.237
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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.QpMFB84F0O (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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=6, blended=1579, bad_region=41, passed=38289
Got 38289 stars (including 36601 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat
util/solve_plate_with_UCAC5 got 38289 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.6'
Seting catalog search parameters based on the expected field of view 943.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013106 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010484 (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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 38289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 38289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4910 matched stars entering correct_measured_positions(), 38289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4910 stars left (next iteration limit 5401)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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=4910 robust_rms=10.630 arcsec worst_region_rms=26.345 arcsec outer_annulus_rms=26.345 arcsec
SIP_REFIT: SIP order 3 trial: matched=4910 robust_rms=0.646 arcsec worst_region_rms=0.892 arcsec outer_annulus_rms=0.892 arcsec
SIP_REFIT: SIP order 5 trial: matched=4910 robust_rms=0.421 arcsec worst_region_rms=0.538 arcsec outer_annulus_rms=0.538 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4910 robust_rms_before=1.179 arcsec robust_rms_before_corrected=0.312 arcsec robust_rms_after=0.421 arcsec worst_region_rms_before=0.456 worst_region_rms_after=0.538 outer_annulus_rms_before=1.296 outer_annulus_rms_after=0.538
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.456 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits worst_region_rms_kept=0.456 arcsec robust_rms_kept=0.312 arcsec matched=4910
WCS_QUALITY_DIAG: file=fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits N_match=4910 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.363 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.357 n_q1=1488 n_q2=940 n_q3=1521 n_q4=961 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-21-44_20.00sec_-0.00C_LIGHTs_0426.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.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_2026-10-10_CI_Cnc-02-Q1b1x1_033826_TTUQ1b1x1_464113_KCGs7tCU/wcs_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427.fits
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:09:40.79 +21:18:10.2: 13.43 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:51:43.77 +20:16:23.3: 12.91 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:54:39.04 +21:14:44.2: 14.38 +/- 0.07 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:21:18.14 +21:45:41.1: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 07:51:43.77 +20:16:23.3: 12.82 +/- 0.02 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 07:54:39.04 +21:14:44.2: 14.33 +/- 0.08 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:09:40.79 +21:18:10.2: 13.40 +/- 0.03 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 07:57:54.80 +23:50:13.9: 16.17 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.86 +/- 0.02
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry reference-image weighted average: 13.42 +/- 0.02
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:38:34.50 +25:23:05.9: 16.12 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 07:51:43.77 +20:16:23.3: ref_mag=12.86 +/- 0.02 new_mean_mag=12.7901 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:54:39.04 +21:14:44.2: ref_mag=14.35 +/- 0.05 new_mean_mag=14.1876 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:09:40.79 +21:18:10.2: ref_mag=13.42 +/- 0.02 new_mean_mag=13.0815 delta=0.34 (need > 0.90)
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:21:18.14 +21:45:41.1: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:05:21.00 +20:16:02.2: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:16:58.68 +19:54:45.2: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 07:57:54.80 +23:50:13.9: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:38:34.50 +25:23:05.9: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:05:21.00 +20:16:02.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:16:58.68 +19:54:45.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits at 08:28:24.87 +19:35:44.9: 10.66 +/- 0.00 detection
Forced photometry on wcs_Cnc-02-Q1b1x1_2026-03-20_23-33-35_20.00sec_-14.90C_LIGHT_0166.fits at 08:28:24.87 +19:35:44.9: 10.61 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.64 +/- 0.00
Forced photometry filter KEPT candidate at 08:28:24.87 +19:35:44.9: ref_mag=10.64 +/- 0.00 new_mean_mag=9.7141 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out22377.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99990.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: 5s
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Considering the candidate 98895_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98895_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 98906_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98906_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:23:51.15 +23:10:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98908_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98908_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:02:03.42 +24:56:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98910_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98910_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 98911_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98911_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:49:03.32 +19:35:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98913_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 98913_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
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Considering the candidate 98914_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 98914_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 99018_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99018_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:21:33.74 +19:25:58.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 99026_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99026_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:57:09.54 +21:19:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99223_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99223_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:28:31.18 +24:09:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99408_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99408_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:36:04.64 +24:01:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99489_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 99489_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 99563_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99563_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:49:10.85 +18:02:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99577_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99577_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:02:18.84 +23:00:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99586_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99586_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:07:25.76 +19:47:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99602_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99602_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:28:42.06 +24:09:17.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99645_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99645_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:40:27.08 +19:39:22.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 99749_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 99749_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 99774_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 99774_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 99818_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99818_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:54:03.37 +19:14:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99897_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 99897_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:31:12.77 +24:25:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99923_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 99923_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 99990_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 99990_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 09274_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 09274_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:44:40.88 +18:09:09.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 19915_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 19915_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:27:40.48 +19:15:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38960_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 38960_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:09:41.10 +21:17:41.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 78986_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 78986_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:10:29.44 +24:01:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23385_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 23385_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:53:43.44 +19:16:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33814_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 33814_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 07:59:14.46 +20:38:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84191_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 84191_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
**** FOUND 08:17:55.92 +23:27:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22377_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
Preparing report for the candidate 22377_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
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Considering the candidate 28047_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427
The candidate 28047_fd_Cnc-02-Q1b1x1_2026-10-10_03-22-40_20.00sec_0.00C_LIGHTs_0427 did not pass the final checks
