This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 12.45 09:21:27.86 +20:23:44.7
209.08938 41.82150 galactic Cnc Second-epoch detections are separated by 1.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.196 Philomela -0 -1 1 12.8 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:27.86 +20:23:44.7: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:27.86 +20:23:44.7: 16.16 +/- 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,2461295.9534,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.4534 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 12.40 09:45:13.38 +22:33:07.2
208.51941 47.74004 galactic Leo Second-epoch detections are separated by 0.7" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.471 Papagena -0 1 1 12.0 0 -0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:45:13.38 +22:33:07.2: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:45:13.38 +22:33:07.2: 15.93 +/- 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!
TCP 2026 09 12.4534* 09 45 13.38 +22 33 07.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461295.9534,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.4534 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.46 09:07:29.38 +23:30:46.3
203.87390 39.67433 galactic Cnc Second-epoch detections are separated by 0.8" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.134 Sophrosyne 1 1 1 14.1 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:07:29.38 +23:30:46.3: 15.66 +/- 0.22 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:07:29.38 +23:30:46.3: 16.10 +/- 0.33 detection
Forced photometry reference-image weighted average: 15.79 +/- 0.18
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,2461295.9534,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.4534 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.46 09:13:03.76 +23:30:50.9
204.34642 40.90000 galactic Cnc Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.87 Sylvia -1 -0 1 13.7 0 -0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:13:03.76 +23:30:50.9: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:13:03.76 +23:30:50.9: 16.27 +/- 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,2461295.9534,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.4534 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.46 09:06:58.27 +20:18:21.4
207.76222 38.57783 galactic Cnc Second-epoch detections are separated by 0.3" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.245 Vera -0 1 1 13.9 -0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:06:58.27 +20:18:21.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:06:58.27 +20:18:21.4: 16.14 +/- 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,2461295.9534,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260912.4534 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.72 09:12:21.12 +17:20:34.4
211.88677 38.75301 galactic Cnc Second-epoch detections are separated by 0.8" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.487 Venetia 1 -1 1 13.9 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:12:21.12 +17:20:34.4: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:12:21.12 +17:20:34.4: 16.05 +/- 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,2461295.9534,13.72,0.05,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 20260912.4534 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.70 09:04:51.82 +18:56:50.9
209.17727 37.65459 galactic Cnc Second-epoch detections are separated by 0.1" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.104 Klymene -0 0 0 14.2 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:04:51.82 +18:56:50.9: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:04:51.82 +18:56:50.9: 16.21 +/- 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,2461295.9534,13.70,0.05,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 20260912.4534 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 12.4534 2461295.9534 13.98 09:07:18.61 +19:01:25.3
209.33819 38.22397 galactic Cnc Second-epoch detections are separated by 1.8" and 3.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.351 Yrsa 0 2 2 14.3 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:07:18.61 +19:01:25.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:07:18.61 +19:01:25.3: 16.16 +/- 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,2461295.9534,13.98,0.05,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 20260912.4534 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461295.95364749 12.09.2026 10:53:05.143 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 4 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): 8754
Objects passed selection criteria: 8728
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: 6715.5
Average stars matched: 6522 (97.1186 %)
Memory usage VmPeak: 241100 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 27 00:41:22 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: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461295.95364749 12.09.2026 10:53:05.143 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 105
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.04
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: 13 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): 47772
Objects passed selection criteria: 47635
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: 38087
Average stars matched: 36786.5 (96.5854 %)
Memory usage VmPeak: 269056 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Sep 27 00:42:09 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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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: 2461295.95311830
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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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: 09:13:50.704 +21:59:59.79 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-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Image size: 945.2'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:55.284 +21:57:40.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:55.284 +21:57:40.63
Angular distance between the image centers 0.0425 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:54.802 +21:57:21.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:54.802 +21:57:21.00
Angular distance between the image centers 0.0469 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 09:13:55.284 +21:57:40.63
Second-epoch second image center 09:13:54.802 +21:57:21.00
Angular distance between the image centers 0.00576 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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.ZFdil2xu2S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.a3WATJdvdc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits &> /tmp/tmp.fJhyH5tyju
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits &> /tmp/tmp.ex8HQgamnL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0580 deg, Dec +16.3325 to +27.3464 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 129.4936 to 147.0580 deg, Dec 16.3325 to 27.3464 deg
Loaded 6006 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): 4510 out of 4801 total matches.
Matched with Tycho-2 4801 out of 9058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920200
a=0.000000 b=1.000000 c=22.920200
From vast_summary.log: estimated ref. image limiting mag.: -7.30
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 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0580 deg, Dec +16.3325 to +27.3464 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 129.4936 to 147.0580 deg, Dec 16.3325 to 27.3464 deg
Loaded 6006 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): 4510 out of 4801 total matches.
Matched with Tycho-2 4801 out of 9058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=6.3)
Read 9037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0623 deg, Dec +16.3327 to +27.3523 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 129.4936 to 147.0623 deg, Dec 16.3327 to 27.3523 deg
Loaded 6008 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): 4486 out of 4794 total matches.
Matched with Tycho-2 4794 out of 9037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Limiting magnitude estimates:
15.6 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.6 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
14.5 mag. fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
14.5 mag. fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.5 (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.ZFdil2xu2S (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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=691, bad_region=0, passed=9058
Got 9058 stars (including 8360 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 9058 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 27.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 9058 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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 9058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 9058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4812 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=4812 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.329 n_q1=1361 n_q2=1105 n_q3=1319 n_q4=1027 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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.a3WATJdvdc (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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=724, bad_region=0, passed=9037
Got 9037 stars (including 8310 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 9037 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 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 4814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4814 stars left (next iteration limit 5295)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=4814 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.362 n_q1=1349 n_q2=1112 n_q3=1325 n_q4=1028 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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.fJhyH5tyju (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.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=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=317, bad_region=0, passed=4456
Got 4456 stars (including 4132 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat
util/solve_plate_with_UCAC5 got 4456 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.2'
Seting catalog search parameters based on the expected field of view 945.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013128 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010502 (37.8 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 3994 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3985 matched stars entering correct_measured_positions(), 3985 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3985 matched stars entering correct_measured_positions(), 4456 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 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 3994 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3986 matched stars entering correct_measured_positions(), 4456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 3986 matched stars entering correct_measured_positions(), 4456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 3986 stars left (next iteration limit 4383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3986 robust_rms=10.846 arcsec worst_region_rms=17.750 arcsec outer_annulus_rms=17.750 arcsec
SIP_REFIT: SIP order 3 trial: matched=3986 robust_rms=0.549 arcsec worst_region_rms=0.754 arcsec outer_annulus_rms=0.754 arcsec
SIP_REFIT: SIP order 5 trial: matched=3986 robust_rms=0.323 arcsec worst_region_rms=0.410 arcsec outer_annulus_rms=0.377 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3986 robust_rms_before=1.486 arcsec robust_rms_before_corrected=0.305 arcsec robust_rms_after=0.323 arcsec worst_region_rms_before=0.386 worst_region_rms_after=0.410 outer_annulus_rms_before=1.657 outer_annulus_rms_after=0.377
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.386 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits worst_region_rms_kept=0.386 arcsec robust_rms_kept=0.305 arcsec matched=3986
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits N_match=3986 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.327 n_q1=1245 n_q2=753 n_q3=1226 n_q4=762 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.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.ex8HQgamnL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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=397, bad_region=0, passed=4568
Got 4568 stars (including 4167 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat
util/solve_plate_with_UCAC5 got 4568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 4019 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4011 matched stars entering correct_measured_positions(), 4011 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4011 matched stars entering correct_measured_positions(), 4568 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 4020 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4012 matched stars entering correct_measured_positions(), 4568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4012 matched stars entering correct_measured_positions(), 4568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4012 stars left (next iteration limit 4412)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4012 robust_rms=10.824 arcsec worst_region_rms=17.835 arcsec outer_annulus_rms=17.835 arcsec
SIP_REFIT: SIP order 3 trial: matched=4012 robust_rms=0.569 arcsec worst_region_rms=0.795 arcsec outer_annulus_rms=0.795 arcsec
SIP_REFIT: SIP order 5 trial: matched=4012 robust_rms=0.348 arcsec worst_region_rms=0.425 arcsec outer_annulus_rms=0.376 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4012 robust_rms_before=1.527 arcsec robust_rms_before_corrected=0.307 arcsec robust_rms_after=0.348 arcsec worst_region_rms_before=0.376 worst_region_rms_after=0.425 outer_annulus_rms_before=1.674 outer_annulus_rms_after=0.376
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.376 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits worst_region_rms_kept=0.376 arcsec robust_rms_kept=0.307 arcsec matched=4012
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits N_match=4012 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.314 n_q1=1263 n_q2=751 n_q3=1231 n_q4=767 worst_quadrant_to_overall_ratio=1.198
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
Saving the final (post-refit) wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
Saving the final (post-refit) wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits'
Saving the final (post-refit) wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits sigma_overall=0.373 worst_q_ratio=1.245
ref2=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits sigma_overall=0.398 worst_q_ratio=1.221
new1=fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits sigma_overall=0.314 worst_q_ratio=1.215
new2=fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits sigma_overall=0.320 worst_q_ratio=1.198
reference average sigma_overall=0.3855 worst_q_ratio=1.233
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199_astrometric_residuals.png (4812 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200_astrometric_residuals.png (4814 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512_astrometric_residuals.png (3986 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513_astrometric_residuals.png (4012 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06162_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 06162_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:02:40.02 +23:54:57.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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: 09:13:50.704 +21:59:59.79 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-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Image size: 945.2'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:55.284 +21:57:40.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:55.284 +21:57:40.63
Angular distance between the image centers 0.0425 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Image size: 945.1'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:54.802 +21:57:21.00 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:54.802 +21:57:21.00
Angular distance between the image centers 0.0469 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 09:13:55.284 +21:57:40.63
Second-epoch second image center 09:13:54.802 +21:57:21.00
Angular distance between the image centers 0.00576 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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.ujf7K7bcpN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.chuI042NiQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits &> /tmp/tmp.jl5qUwghOk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits &> /tmp/tmp.UBNAf7bKko
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0734 deg, Dec +16.3325 to +27.3500 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 129.4936 to 147.0734 deg, Dec 16.3325 to 27.3500 deg
Loaded 6016 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): 4201 out of 4841 total matches.
Matched with Tycho-2 4841 out of 50507 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.814600
a=0.000000 b=1.000000 c=22.814600
From vast_summary.log: estimated ref. image limiting mag.: -7.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0734 deg, Dec +16.3325 to +27.3500 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 129.4936 to 147.0734 deg, Dec 16.3325 to 27.3500 deg
Loaded 6016 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): 4201 out of 4841 total matches.
Matched with Tycho-2 4841 out of 50507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=5.0)
Read 50709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4911 to 147.0623 deg, Dec +16.3281 to +27.3564 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 129.4911 to 147.0623 deg, Dec 16.3281 to 27.3564 deg
Loaded 6019 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): 4178 out of 4842 total matches.
Matched with Tycho-2 4842 out of 50709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 96 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Limiting magnitude estimates:
15.8 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.8 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
14.6 mag. fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
14.6 mag. fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (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.ujf7K7bcpN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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=25, blended=2848, bad_region=9, passed=50482
Got 50482 stars (including 47524 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 50482 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 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4811 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=4811 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.320 n_q1=1326 n_q2=1103 n_q3=1308 n_q4=1074 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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.chuI042NiQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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=29, blended=2904, bad_region=11, passed=50680
Got 50680 stars (including 47683 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 50680 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 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 50680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 50680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 50680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4815 stars left (next iteration limit 5297)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=4815 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.346 n_q1=1321 n_q2=1100 n_q3=1315 n_q4=1079 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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.jl5qUwghOk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.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=8, blended=911, bad_region=15, passed=26103
Got 26103 stars (including 25136 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat
util/solve_plate_with_UCAC5 got 26103 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.2'
Seting catalog search parameters based on the expected field of view 945.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013128 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010502 (37.8 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 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 26103 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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 26103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 26103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4813 stars left (next iteration limit 5293)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.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=4813 robust_rms=10.349 arcsec worst_region_rms=17.726 arcsec outer_annulus_rms=17.726 arcsec
SIP_REFIT: SIP order 3 trial: matched=4813 robust_rms=0.540 arcsec worst_region_rms=0.755 arcsec outer_annulus_rms=0.755 arcsec
SIP_REFIT: SIP order 5 trial: matched=4813 robust_rms=0.326 arcsec worst_region_rms=0.409 arcsec outer_annulus_rms=0.384 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4813 robust_rms_before=1.476 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.326 arcsec worst_region_rms_before=0.378 worst_region_rms_after=0.409 outer_annulus_rms_before=1.616 outer_annulus_rms_after=0.384
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.378 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits worst_region_rms_kept=0.378 arcsec robust_rms_kept=0.303 arcsec matched=4813
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits N_match=4813 sigma_overall_arcsec=0.306 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.359 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.322 n_q1=1545 n_q2=862 n_q3=1498 n_q4=908 worst_quadrant_to_overall_ratio=1.174
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.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.UBNAf7bKko (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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=5, blended=1160, bad_region=17, passed=26301
Got 26301 stars (including 25090 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat
util/solve_plate_with_UCAC5 got 26301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.1'
Seting catalog search parameters based on the expected field of view 945.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013126 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010501 (37.8 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 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 4815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 26301 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 530 to 589 (Dec 16.2 to 27.4)
Done reading UCAC5 zone files...
Matched 4825 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 26301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 26301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4815 stars left (next iteration limit 5296)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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=4815 robust_rms=10.309 arcsec worst_region_rms=17.958 arcsec outer_annulus_rms=17.958 arcsec
SIP_REFIT: SIP order 3 trial: matched=4815 robust_rms=0.550 arcsec worst_region_rms=0.799 arcsec outer_annulus_rms=0.799 arcsec
SIP_REFIT: SIP order 5 trial: matched=4815 robust_rms=0.353 arcsec worst_region_rms=0.428 arcsec outer_annulus_rms=0.383 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4815 robust_rms_before=1.522 arcsec robust_rms_before_corrected=0.303 arcsec robust_rms_after=0.353 arcsec worst_region_rms_before=0.378 worst_region_rms_after=0.428 outer_annulus_rms_before=1.619 outer_annulus_rms_after=0.383
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.378 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits worst_region_rms_kept=0.378 arcsec robust_rms_kept=0.303 arcsec matched=4815
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits N_match=4815 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.289 sigma_q4_arcsec=0.308 n_q1=1556 n_q2=859 n_q3=1495 n_q4=905 worst_quadrant_to_overall_ratio=1.236
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.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-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-52-19_20.00sec_-0.00C_LIGHTs_0512.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-09-26_CI_Cnc-03-Q1b1x1_222631_TTUQ1b1x1_628393_A1Xxj2ll/wcs_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:21:27.86 +20:23:44.7: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:09:13.13 +22:04:11.6: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:45:13.38 +22:33:07.2: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:46:26.78 +17:30:59.5: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:04:51.15 +24:37:33.8: 13.32 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:46:15.68 +20:36:40.3: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:21:27.86 +20:23:44.7: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:09:13.13 +22:04:11.6: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter REJECTED candidate at 09:09:13.13 +22:04:11.6: ref_mag=12.90 +/- 0.01 new_mean_mag=12.8194 delta=0.08 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:45:13.38 +22:33:07.2: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:46:26.78 +17:30:59.5: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 08:46:26.78 +17:30:59.5: ref_mag=13.16 +/- 0.02 new_mean_mag=13.0946 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:04:51.15 +24:37:33.8: 13.30 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.31 +/- 0.02
Forced photometry filter REJECTED candidate at 09:04:51.15 +24:37:33.8: ref_mag=13.31 +/- 0.02 new_mean_mag=13.1961 delta=0.12 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:46:15.68 +20:36:40.3: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter REJECTED candidate at 08:46:15.68 +20:36:40.3: ref_mag=13.60 +/- 0.03 new_mean_mag=13.5012 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:07:29.38 +23:30:46.3: 15.66 +/- 0.22 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:07:29.38 +23:30:46.3: 16.10 +/- 0.33 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:13:03.76 +23:30:50.9: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:06:58.27 +20:18:21.4: 16.14 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.79 +/- 0.18
Forced photometry filter KEPT candidate at 09:07:29.38 +23:30:46.3: ref_mag=15.79 +/- 0.18 new_mean_mag=13.4533 delta=2.34 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:12:21.12 +17:20:34.4: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:06:58.27 +20:18:21.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:13:03.76 +23:30:50.9: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:54:38.87 +24:12:08.2: 14.23 +/- 0.07 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:12:21.12 +17:20:34.4: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:04:51.82 +18:56:50.9: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:54:38.87 +24:12:08.2: 14.19 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.21 +/- 0.05
Forced photometry filter REJECTED candidate at 08:54:38.87 +24:12:08.2: ref_mag=14.21 +/- 0.05 new_mean_mag=14.0705 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:04:51.82 +18:56:50.9: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:07:18.61 +19:01:25.3: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:07:18.61 +19:01:25.3: 16.16 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out64628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65231.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 64173_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64173_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 08:43:44.16 +21:35:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64174_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64174_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 08:43:04.96 +19:27:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64253_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64253_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 64277_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64277_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64278_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64278_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 64345_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64345_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64363_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64363_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 64391_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64391_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 64396_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64396_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64429_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64429_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64432_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64432_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 64484_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64484_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64503_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64503_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 64514_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64514_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 64523_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64523_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 64524_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64524_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64545_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64545_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 64552_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64552_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 64553_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64553_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:09:53.97 +25:12:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64615_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64615_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 08:57:14.48 +17:08:08.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 64628_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 64628_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 64651_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64651_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 64657_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64657_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64669_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64669_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:01:45.98 +17:06:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64678_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64678_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64681_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64681_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
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Considering the candidate 64684_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64684_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64688_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64688_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:04:57.36 +24:36:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64696_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 64696_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 64698_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64698_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
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Considering the candidate 64740_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64740_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64741_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64741_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 64764_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64764_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 64786_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64786_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64800_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64800_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
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Considering the candidate 64802_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64802_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64814_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64814_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 64823_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64823_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
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Considering the candidate 64825_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64825_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64829_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64829_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 64851_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64851_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64886_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64886_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 08:54:55.82 +26:13:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64908_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64908_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:00:28.64 +22:43:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64913_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64913_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 64916_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64916_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 64918_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64918_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:09:47.16 +25:13:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64924_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64924_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64926_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64926_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:20:35.08 +22:39:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64935_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 64935_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 64947_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64947_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64950_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64950_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 64951_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64951_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 64981_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64981_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 08:49:21.82 +17:58:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64985_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 64985_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:12:51.73 +17:27:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64991_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 64991_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 64999_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 64999_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 65000_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65000_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 65010_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65010_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:16:16.53 +23:25:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65079_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65079_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 65083_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 65083_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 65106_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65106_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 65119_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65119_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 65141_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65141_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 65143_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65143_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 65146_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65146_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 65147_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65147_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:12:47.98 +20:01:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65153_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65153_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
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Considering the candidate 65160_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65160_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 65164_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 65164_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 65165_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65165_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 65183_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65183_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 65190_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65190_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 65201_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65201_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 65212_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65212_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 65216_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65216_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 65231_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
Preparing report for the candidate 65231_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
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Considering the candidate 65233_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65233_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 65243_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65243_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 65249_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65249_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 65254_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65254_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:15:26.89 +23:45:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65262_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65262_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 65272_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65272_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 65274_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65274_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 65276_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65276_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 65280_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65280_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 65286_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65286_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 65294_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65294_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 65297_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65297_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 65303_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65303_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 65312_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65312_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 65313_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65313_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 65317_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 65317_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 06054_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 06054_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:01:03.28 +17:53:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13343_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 13343_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:13:31.87 +19:34:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47832_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 47832_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
**** FOUND 09:02:40.03 +23:54:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04092_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513
The candidate 04092_fd_Cnc-03-Q1b1x1_2026-09-12_05-53-05_20.00sec_0.00C_LIGHTs_0513 did not pass the final checks
