This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD
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 10 21.4549 2461334.9549 12.91 10:49:28.44 +07:15:59.2
241.77508 54.92754 galactic Leo Second-epoch detections are separated by 0.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.45 Eugenia -1 0 1 13.3 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:49:28.44 +07:15:59.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:49:28.44 +07:15:59.2: 15.84 +/- 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 10 21.4549* 10 49 28.44 +07 15 59.2 12.9 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,2461334.9549,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4549 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 12.87 11:10:40.81 +00:58:52.7
255.96703 54.39464 galactic Leo Second-epoch detections are separated by 2.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.32 Pomona -0 -0 0 13.0 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:10:40.81 +00:58:52.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:10:40.81 +00:58:52.7: 15.77 +/- 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 10 21.4549* 11 10 40.81 +00 58 52.7 12.9 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,2461334.9549,12.87,0.05,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 20261021.4549 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 12.96 10:58:05.20 +03:56:18.7
248.55077 54.37095 galactic Leo Second-epoch detections are separated by 1.4" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.43 Ariadne -1 0 1 13.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:58:05.20 +03:56:18.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:58:05.20 +03:56:18.7: 15.85 +/- 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 10 21.4549* 10 58 05.20 +03 56 18.7 13.0 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,2461334.9549,12.96,0.05,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 20261021.4549 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 13.66 10:54:21.22 +04:26:23.6
246.84020 54.02960 galactic Leo Second-epoch detections are separated by 2.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.194 Prokne -1 1 1 14.1 -0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:54:21.22 +04:26:23.6: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:54:21.22 +04:26:23.6: 15.88 +/- 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 10 21.4549* 10 54 21.22 +04 26 23.6 13.7 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,2461334.9549,13.66,0.05,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 20261021.4549 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 13.79 11:11:19.72 +03:22:08.3
253.38955 56.28680 galactic Leo Second-epoch detections are separated by 1.6" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.133 Cyrene -1 1 1 14.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:11:19.72 +03:22:08.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:11:19.72 +03:22:08.3: 15.83 +/- 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 10 21.4549* 11 11 19.72 +03 22 08.3 13.8 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,2461334.9549,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4549 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 13.97 11:19:38.09 +01:11:06.4
258.76709 55.97489 galactic Leo Second-epoch detections are separated by 2.0" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.218 Bianca 2 0 2 14.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:19:38.09 +01:11:06.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:19:38.09 +01:11:06.4: 15.71 +/- 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 10 21.4549* 11 19 38.09 +01 11 06.4 14.0 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,2461334.9549,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261021.4549 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 21.4549 2461334.9549 14.26 11:17:12.58 +07:00:55.8
250.59312 59.92883 galactic Leo Second-epoch detections are separated by 2.9" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.261 Prymno -0 1 1 14.3 0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:12.58 +07:00:55.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:12.58 +07:00:55.8: 15.91 +/- 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 10 21.4549* 11 17 12.58 +07 00 55.8 14.3 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,2461334.9549,14.26,0.05,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 20261021.4549 14.26CV 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: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461334.95525649 21.10.2026 10:55:24.161 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5333
Objects passed selection criteria: 5320
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: 4222.75
Average stars matched: 4113.75 (97.4187 %)
Memory usage VmPeak: 238900 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 05:58:03 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: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461334.95525649 21.10.2026 10:55:24.161 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27180
Objects passed selection criteria: 27114
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 23767.5
Average stars matched: 22826.2 (96.0398 %)
Memory usage VmPeak: 256172 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 05:58:51 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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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: 2461334.95447488
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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.747 +05:57:39.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Image size: 945.4'x627.1' 15.8(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:49.220 +05:59:30.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:49.220 +05:59:30.68
Angular distance between the image centers 0.0438 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Image size: 945.2'x627.1' 15.8(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:46.645 +05:59:00.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:46.645 +05:59:00.20
Angular distance between the image centers 0.0303 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 11:08:49.220 +05:59:30.68
Second-epoch second image center 11:08:46.645 +05:59:00.20
Angular distance between the image centers 0.01362 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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.UKdtqFLj2M
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.tYebHST4TE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits &> /tmp/tmp.S7433Xpj71
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits &> /tmp/tmp.tC0dwTNUWq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1359 to 175.0748 deg, Dec +0.5733 to +11.2587 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 159.1359 to 175.0748 deg, Dec 0.5733 to 11.2587 deg
Loaded 3956 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): 3203 out of 3314 total matches.
Matched with Tycho-2 3314 out of 5626 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.762800
a=0.000000 b=1.000000 c=22.762800
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1359 to 175.0748 deg, Dec +0.5733 to +11.2587 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 159.1359 to 175.0748 deg, Dec 0.5733 to 11.2587 deg
Loaded 3956 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): 3203 out of 3314 total matches.
Matched with Tycho-2 3314 out of 5626 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=6.5)
Read 5579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1762 to 175.0853 deg, Dec +0.7334 to +11.2822 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 159.1762 to 175.0853 deg, Dec 0.7334 to 11.2822 deg
Loaded 3902 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): 3209 out of 3300 total matches.
Matched with Tycho-2 3300 out of 5579 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.3 pix Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.3 pix fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
2.2 pix fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Limiting magnitude estimates:
15.4 mag. Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.3 mag. Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.5 mag. fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
14.5 mag. fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.3 (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.UKdtqFLj2M (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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=364, bad_region=0, passed=5626
Got 5626 stars (including 5255 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 5626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
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: 4806 matched stars entering correct_measured_positions(), 4806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 452 to 508 (Dec 0.6 to 11.3)
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: 4805 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4805 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4805 stars left (next iteration limit 5286)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=4805 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.419 n_q1=1175 n_q2=1236 n_q3=1168 n_q4=1226 worst_quadrant_to_overall_ratio=1.048
WCS_HEADER_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits selection=current_pairs N_selected=4805 N_valid=4805 bias_ra_arcsec=-0.012 bias_dec_arcsec=-0.004 median_sep_arcsec=0.327 p95_sep_arcsec=1.168 n_q1=1175 n_q2=1236 n_q3=1168 n_q4=1226 occupied_cells_4x4=16/16
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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.tYebHST4TE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, bad_region=1, passed=5576
Got 5576 stars (including 5239 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 5576 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4825 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 453 to 508 (Dec 0.7 to 11.3)
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: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4813 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=4813 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.476 n_q1=1150 n_q2=1248 n_q3=1173 n_q4=1242 worst_quadrant_to_overall_ratio=1.139
WCS_HEADER_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits selection=current_pairs N_selected=4813 N_valid=4813 bias_ra_arcsec=-0.023 bias_dec_arcsec=0.005 median_sep_arcsec=0.323 p95_sep_arcsec=1.289 n_q1=1150 n_q2=1248 n_q3=1173 n_q4=1242 occupied_cells_4x4=16/16
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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.S7433Xpj71 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.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=207, bad_region=0, passed=2891
Got 2891 stars (including 2679 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat
util/solve_plate_with_UCAC5 got 2891 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.4'
Seting catalog search parameters based on the expected field of view 945.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013131 (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 0.010504 (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 452 to 509 (Dec 0.5 to 11.4)
Done reading UCAC5 zone files...
Matched 2575 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2565 matched stars entering correct_measured_positions(), 2566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2565 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 452 to 509 (Dec 0.5 to 11.4)
Done reading UCAC5 zone files...
Matched 2574 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2566 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 2566 matched stars entering correct_measured_positions(), 2891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 2566 stars left (next iteration limit 2821)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2566 robust_rms=10.493 arcsec worst_region_rms=20.072 arcsec outer_annulus_rms=20.072 arcsec
SIP_REFIT: SIP order 3 trial: matched=2566 robust_rms=0.623 arcsec worst_region_rms=0.938 arcsec outer_annulus_rms=0.914 arcsec
SIP_REFIT: SIP order 5 trial: matched=2566 robust_rms=0.366 arcsec worst_region_rms=0.455 arcsec outer_annulus_rms=0.349 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2566 robust_rms_before=1.768 arcsec robust_rms_before_corrected=0.353 arcsec robust_rms_after=0.366 arcsec worst_region_rms_before=0.485 worst_region_rms_after=0.455 outer_annulus_rms_before=1.817 outer_annulus_rms_after=0.349
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.485 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits worst_region_rms_kept=0.485 arcsec robust_rms_kept=0.353 arcsec matched=2566
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits N_match=2566 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.332 n_q1=664 n_q2=546 n_q3=732 n_q4=624 worst_quadrant_to_overall_ratio=1.361
WCS_HEADER_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits selection=current_pairs N_selected=2566 N_valid=2566 bias_ra_arcsec=0.911 bias_dec_arcsec=0.408 median_sep_arcsec=1.611 p95_sep_arcsec=3.872 n_q1=664 n_q2=546 n_q3=732 n_q4=624 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.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.tC0dwTNUWq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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=244, bad_region=0, passed=2914
Got 2914 stars (including 2668 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 2914 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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 2562 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2552 matched stars entering correct_measured_positions(), 2553 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2552 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 2561 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2551 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 2551 matched stars entering correct_measured_positions(), 2913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 2551 stars left (next iteration limit 2807)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2551 robust_rms=10.790 arcsec worst_region_rms=19.782 arcsec outer_annulus_rms=19.782 arcsec
SIP_REFIT: SIP order 3 trial: matched=2551 robust_rms=0.651 arcsec worst_region_rms=1.110 arcsec outer_annulus_rms=0.902 arcsec
SIP_REFIT: SIP order 5 trial: matched=2551 robust_rms=0.374 arcsec worst_region_rms=0.479 arcsec outer_annulus_rms=0.404 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2551 robust_rms_before=1.691 arcsec robust_rms_before_corrected=0.353 arcsec robust_rms_after=0.374 arcsec worst_region_rms_before=0.486 worst_region_rms_after=0.479 outer_annulus_rms_before=1.709 outer_annulus_rms_after=0.404
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.486 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits worst_region_rms_kept=0.486 arcsec robust_rms_kept=0.353 arcsec matched=2551
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits N_match=2551 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.473 sigma_q3_arcsec=0.304 sigma_q4_arcsec=0.383 n_q1=641 n_q2=555 n_q3=725 n_q4=630 worst_quadrant_to_overall_ratio=1.313
WCS_HEADER_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits selection=current_pairs N_selected=2551 N_valid=2551 bias_ra_arcsec=0.922 bias_dec_arcsec=0.427 median_sep_arcsec=1.537 p95_sep_arcsec=3.623 n_q1=641 n_q2=555 n_q3=725 n_q4=630 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
Saving the final (post-refit) wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
Saving the final (post-refit) wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits'
Saving the final (post-refit) wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits sigma_overall=0.413 worst_q_ratio=1.048
ref2=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits sigma_overall=0.418 worst_q_ratio=1.139
new1=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits sigma_overall=0.361 worst_q_ratio=1.361
new2=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits sigma_overall=0.360 worst_q_ratio=1.313
reference average sigma_overall=0.4155 worst_q_ratio=1.0935
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503_astrometric_residuals.png (4805 matched stars from wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148_astrometric_residuals.png (4813 matched stars from wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470_astrometric_residuals.png (2566 matched stars from wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471_astrometric_residuals.png (2551 matched stars from wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits'
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-07-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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.747 +05:57:39.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Image size: 945.4'x627.1' 15.8(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:49.220 +05:59:30.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:49.220 +05:59:30.68
Angular distance between the image centers 0.0438 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Image size: 945.2'x627.1' 15.8(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:46.645 +05:59:00.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:46.645 +05:59:00.20
Angular distance between the image centers 0.0303 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 11:08:49.220 +05:59:30.68
Second-epoch second image center 11:08:46.645 +05:59:00.20
Angular distance between the image centers 0.01362 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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.Hk5nSr1gOd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.HqEVpUnArq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits &> /tmp/tmp.lDspBlbgWp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits &> /tmp/tmp.8tnRpzxncP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1348 to 175.0760 deg, Dec +0.5733 to +11.2606 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 159.1348 to 175.0760 deg, Dec 0.5733 to 11.2606 deg
Loaded 3958 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): 3142 out of 3395 total matches.
Matched with Tycho-2 3395 out of 29706 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.644650
a=0.000000 b=1.000000 c=22.644650
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1348 to 175.0760 deg, Dec +0.5733 to +11.2606 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 159.1348 to 175.0760 deg, Dec 0.5733 to 11.2606 deg
Loaded 3958 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): 3142 out of 3395 total matches.
Matched with Tycho-2 3395 out of 29706 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=5.1)
Read 29098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1762 to 175.0872 deg, Dec +0.7305 to +11.2848 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 159.1762 to 175.0872 deg, Dec 0.7305 to 11.2848 deg
Loaded 3903 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): 3155 out of 3382 total matches.
Matched with Tycho-2 3382 out of 29098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.2 pix Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.2 pix fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Limiting magnitude estimates:
15.5 mag. Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.5 mag. Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.7 mag. fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
14.7 mag. fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
All-image limiting magnitude estimate: 14.7 (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.Hk5nSr1gOd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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=20, blended=1187, bad_region=0, passed=29686
Got 29686 stars (including 28458 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 29686 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4798 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=4798 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.410 n_q1=1127 n_q2=1275 n_q3=1148 n_q4=1248 worst_quadrant_to_overall_ratio=1.035
WCS_HEADER_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits selection=current_pairs N_selected=4798 N_valid=4798 bias_ra_arcsec=-0.039 bias_dec_arcsec=0.001 median_sep_arcsec=0.324 p95_sep_arcsec=1.167 n_q1=1127 n_q2=1275 n_q3=1148 n_q4=1248 occupied_cells_4x4=16/16
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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.HqEVpUnArq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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=17, blended=1226, bad_region=1, passed=29081
Got 29081 stars (including 27822 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 29081 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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: 4809 matched stars entering correct_measured_positions(), 4809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 29081 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 453 to 508 (Dec 0.7 to 11.3)
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: 4809 matched stars entering correct_measured_positions(), 29081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 29081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4809 stars left (next iteration limit 5289)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=4809 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.444 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.449 n_q1=1165 n_q2=1236 n_q3=1196 n_q4=1212 worst_quadrant_to_overall_ratio=1.130
WCS_HEADER_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits selection=current_pairs N_selected=4809 N_valid=4809 bias_ra_arcsec=-0.029 bias_dec_arcsec=0.012 median_sep_arcsec=0.315 p95_sep_arcsec=1.197 n_q1=1165 n_q2=1236 n_q3=1196 n_q4=1212 occupied_cells_4x4=16/16
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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.lDspBlbgWp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.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=3, blended=738, bad_region=38, passed=18617
Got 18617 stars (including 17800 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat
util/solve_plate_with_UCAC5 got 18617 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.4'
Seting catalog search parameters based on the expected field of view 945.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013131 (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 0.010504 (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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 4769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 18617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 18617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4769 matched stars entering correct_measured_positions(), 18617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4769 stars left (next iteration limit 5244)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.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=4769 robust_rms=10.099 arcsec worst_region_rms=22.125 arcsec outer_annulus_rms=22.125 arcsec
SIP_REFIT: SIP order 3 trial: matched=4769 robust_rms=0.644 arcsec worst_region_rms=0.923 arcsec outer_annulus_rms=0.923 arcsec
SIP_REFIT: SIP order 5 trial: matched=4769 robust_rms=0.401 arcsec worst_region_rms=0.491 arcsec outer_annulus_rms=0.416 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4769 robust_rms_before=1.754 arcsec robust_rms_before_corrected=0.358 arcsec robust_rms_after=0.401 arcsec worst_region_rms_before=0.449 worst_region_rms_after=0.491 outer_annulus_rms_before=1.731 outer_annulus_rms_after=0.416
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.449 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits worst_region_rms_kept=0.449 arcsec robust_rms_kept=0.358 arcsec matched=4769
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits N_match=4769 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.462 sigma_q3_arcsec=0.341 sigma_q4_arcsec=0.358 n_q1=1330 n_q2=989 n_q3=1356 n_q4=1094 worst_quadrant_to_overall_ratio=1.269
WCS_HEADER_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits selection=current_pairs N_selected=4769 N_valid=4769 bias_ra_arcsec=0.916 bias_dec_arcsec=0.396 median_sep_arcsec=1.599 p95_sep_arcsec=3.713 n_q1=1330 n_q2=989 n_q3=1356 n_q4=1094 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.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.8tnRpzxncP (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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=531, bad_region=39, passed=18566
Got 18566 stars (including 17969 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat
util/solve_plate_with_UCAC5 got 18566 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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 4785 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 4769 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4768 matched stars entering correct_measured_positions(), 18566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 452 to 509 (Dec 0.4 to 11.4)
Done reading UCAC5 zone files...
Matched 4785 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 18566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4770 matched stars entering correct_measured_positions(), 18566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4770 stars left (next iteration limit 5244)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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=4770 robust_rms=10.340 arcsec worst_region_rms=22.440 arcsec outer_annulus_rms=22.440 arcsec
SIP_REFIT: SIP order 3 trial: matched=4770 robust_rms=0.664 arcsec worst_region_rms=1.026 arcsec outer_annulus_rms=0.930 arcsec
SIP_REFIT: SIP order 5 trial: matched=4770 robust_rms=0.410 arcsec worst_region_rms=0.512 arcsec outer_annulus_rms=0.449 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4770 robust_rms_before=1.684 arcsec robust_rms_before_corrected=0.360 arcsec robust_rms_after=0.410 arcsec worst_region_rms_before=0.450 worst_region_rms_after=0.512 outer_annulus_rms_before=1.675 outer_annulus_rms_after=0.449
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.450 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits worst_region_rms_kept=0.450 arcsec robust_rms_kept=0.360 arcsec matched=4770
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits N_match=4770 sigma_overall_arcsec=0.365 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.453 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.347 n_q1=1328 n_q2=1002 n_q3=1350 n_q4=1090 worst_quadrant_to_overall_ratio=1.240
WCS_HEADER_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits selection=current_pairs N_selected=4770 N_valid=4770 bias_ra_arcsec=0.915 bias_dec_arcsec=0.409 median_sep_arcsec=1.537 p95_sep_arcsec=3.538 n_q1=1328 n_q2=1002 n_q3=1350 n_q4=1090 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.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_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-54-16_20.00sec_-0.00C_LIGHTs_0470.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Leo-07-Q1b1x1_055612_TTUQ1b1x1_3999926_WNfz5AtD/wcs_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471.fits
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:38:16.64 +08:24:37.3: 13.77 +/- 0.06 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:19:21.06 +08:16:49.2: 13.87 +/- 0.06 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:58:05.20 +03:56:18.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:49:28.44 +07:15:59.2: 15.89 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:10:40.81 +00:58:52.7: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:48.32 +03:51:38.0: 13.06 +/- 0.03 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:51:31.59 +05:28:01.2: 13.41 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:39:45.10 +06:01:49.3: 13.37 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:52:04.24 +08:52:04.6: 13.40 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:49:28.44 +07:15:59.2: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:51:31.59 +05:28:01.2: 13.55 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:48.32 +03:51:38.0: 13.00 +/- 0.03 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:19:21.06 +08:16:49.2: 13.68 +/- 0.05 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:58:05.20 +03:56:18.7: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:10:40.81 +00:58:52.7: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:38:16.64 +08:24:37.3: 13.76 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.03
Forced photometry reference-image weighted average: 13.03 +/- 0.02
Forced photometry reference-image weighted average: 13.76 +/- 0.04
Forced photometry filter REJECTED candidate at 10:51:31.59 +05:28:01.2: ref_mag=13.47 +/- 0.03 new_mean_mag=13.6101 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:17:48.32 +03:51:38.0: ref_mag=13.03 +/- 0.02 new_mean_mag=13.2439 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:19:21.06 +08:16:49.2: ref_mag=13.76 +/- 0.04 new_mean_mag=13.7236 delta=0.04 (need > 0.90)
Forced photometry reference-image weighted average: 13.77 +/- 0.04
Forced photometry filter REJECTED candidate at 10:38:16.64 +08:24:37.3: ref_mag=13.77 +/- 0.04 new_mean_mag=13.7473 delta=0.02 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:39:45.10 +06:01:49.3: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.36 +/- 0.03
Forced photometry filter REJECTED candidate at 10:39:45.10 +06:01:49.3: ref_mag=13.36 +/- 0.03 new_mean_mag=13.3906 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:52:04.24 +08:52:04.6: 13.51 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.45 +/- 0.03
Forced photometry filter REJECTED candidate at 10:52:04.24 +08:52:04.6: ref_mag=13.45 +/- 0.03 new_mean_mag=13.5564 delta=-0.11 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:54:21.22 +04:26:23.6: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:11:19.72 +03:22:08.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:38:22.41 +02:31:40.4: 14.00 +/- 0.08 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:19:38.09 +01:11:06.4: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:12.58 +07:00:55.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:54:21.22 +04:26:23.6: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:38:22.41 +02:31:40.4: 14.02 +/- 0.09 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:11:19.72 +03:22:08.3: 15.83 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.01 +/- 0.06
Forced photometry filter REJECTED candidate at 10:38:22.41 +02:31:40.4: ref_mag=14.01 +/- 0.06 new_mean_mag=13.8538 delta=0.16 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:19:38.09 +01:11:06.4: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:12.58 +07:00:55.8: 15.91 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out32704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33370.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32454_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32454_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 10:42:19.93 +08:08:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32456_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32456_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32460_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32460_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32461_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32461_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32462_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32462_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32464_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32464_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 10:38:36.80 +02:35:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32633_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32633_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 10:40:59.64 +05:47:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32704_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 32704_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32753_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 32753_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32766_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 32766_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32780_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32780_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32849_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32849_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 11:28:23.93 +09:24:27.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32864_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32864_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32998_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 32998_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 11:36:35.00 +06:07:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33014_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 33014_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 11:21:16.91 +06:01:25.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33019_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 33019_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33088_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 33088_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 11:04:58.15 +07:22:12.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33090_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 33090_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33215_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 33215_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33353_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 33353_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33370_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
Preparing report for the candidate 33370_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12649_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 12649_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
**** FOUND 10:59:40.37 +06:37:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15183_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471
The candidate 15183_fd_Leo-07-Q1b1x1_2026-10-21_05-55-24_20.00sec_0.00C_LIGHTs_0471 did not pass the final checks
